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2004 Ams Nim Paper Draft

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Page 1: 2004 Ams Nim Paper Draft

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Page 2: 2004 Ams Nim Paper Draft
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AMS on ISS Construction of a particle physics detector

on the International Space Station

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(121!(#3045!'1!6)775!"#1!8/-05!91!8+-7/0:;/5!81!<=,$*:>$?$-5!'1!'@#+$*5!%1!'@#3*.A!B)0!C-+.A/45!D1!'@#E$-/045!"#1!'/$F$0,3-45!G1!'/$F*/045!91!9+**-+HH5!&1!9*)@#+*!

I. Physikalisches Institut, RWTH, D-52056 Aachen, Germany !

21IJ1!J-)$;$-5!K1!()>>/@#+35!D1!6*3$44$5!81!2+04+-.$-!III. Physikalisches Institut, RWTH, D-52056 Aachen, Germany

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L$:!&+F:$0!Department of Physics and Astronomy, University of Aarhus, DK-8000 Aarhus C, Denmark

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21!J)$-!G));#3/A$05!(1!'0/77$5!J1!K$-*++.!National Institute for Nuclear Physics and High Energy Physics, NIKHEF, NL-1098 SJ Amsterdam,

The Netherlands !

(1!%F*)HH5!61!(+F)3M5!D1!()/40$.5!<1!D/-+-F5!(1!D)?5!G1!2$->$*5!G1!8)::+;)E:;/!5!L1!N)@#)05!!'1!G):/$-I<$$:5!L1IN1!K/+**$!

Laboratoire d'Annecy-le-Vieux de Physique des Particules, LAPP, F-74941 Annecy-le-Vieux CEDEX, France !

%1!N$B:0$-!Johns Hopkins University, Baltimore, MD 21218, USA

!

'1J1!J+/5!O1P1!6$045!61!D+)5!Q1L1!2+05!81!<3)5!61Q1!'#$05!G121!9$/5!'121!Q/+045!<1L1!Q35!'1!O+045!R121!R#3!

Beijing Institute of Spacecraft Environment Engineering, BISEE, 100029 Beijing, China !

R1D1!(#$05!(1&1!</5!S1!</5!Q1J1!N$045!L1D1!"+04!Chinese Academy of Launching Vehicle Technology, CALT, 100076 Beijing, China

!O1&1!C+/5!S121!')045!P1<1!9+045!O1L1!O3

Institute of Electrical Engineering, IEE, Chinese Academy of Sciences, 100080 Beijing, China

!D1&1!(#$05!21'1!(#$05!R121!</5!O1'1!<35!Q191!"+045!(1D1!O+045!&1!O+045!R1P1!O35!21<1!R#3+04!!

Institute of High Energy Physics, IHEP, Chinese Academy of Sciences, 100039 Beijing, China

!&1!J+:/*$TU5VU5!K1!J/0F/TU5VU5!C1!(+:+F$/TU5VU5!61!(/0F)*)TU5!%1!()0./0TU5VU5!%1!WB+04$*/:.+TU5!'1!6/0$**/TU5!

61!D/)B+@@#/0/TU5VU5!(1!D3+0F+*/0/TU5!D1!<+3-$0./TU5!D1!<$B/TU5VU5!&1!<)**/TU5!G1!&+-.$**/TU5VU5!<1!P3+F-+0/TU5VU5!61!N+*>)0+-/TU5VU5!D1!'+-.)-$**/TU5VU5!(1!',+--+TU5VU5!%1!R/@#/@#/TU5VU5!%1!R3@@#/0/TU!

University of Bologna and INFN-Sezione di Bologna, I-40126 Bologna, Italy TU!INFN-Sezione di Bologna,!

VU!Universita’ di Bologna!

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S1!C/03TU5!&1!X)0/@+VU5!G1!X)0/@+YU5!61!&+0)*$:@3TU5!Z1!&+-/:TU5!%1!&/#3*[U!Institute of Microtechnology, Institute for Space Sciences and University of Bucharest, R-76900 Bucharest,

Romania TU Institute for Space Science, ISS, VU Institute for Microtechnology, IMT, YU University Politechnica, UPB, [U University of Bucharest, UB

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G1!J$@;$-5!\1!J$@;$-5!N1!J$-4$:5!L1C1!J3-4$-5!Q1C1!(+/5!&1!(+7$**5!D1!(+-):/5!K1!(#)3.;)5!J1!C$>/-;)A5!N1!C$00$..5!61L1!W77*/045!N121!6/:#$-5!%1!8*/>$0.)B5!%1!8)3*$>A/0$5!%1!8)30/0$5!K1!8)3.:$0;)5!

%1!<$,$F$B5!J1!&)0-$+*5!%1!G)A#;)B5!81!'@#)*,$-45!'+>3$*!(1(1!"/045!'1&1!"/045!&1!'.$3$-5!'1!Q/+)5!'1C1!Q35!&1!K$-4+/05!O1!9+045!Q1R1!9+04!

Massachusetts Institute of Technology, MIT, Cambridge, MA 02139, USA !

O121!(#+045!(121!</0!National Central University, Chung-Li, Taiwan 32054

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%1!&+*/0/0$5!W1I'1!'$)!IPST, University of Maryland, College Park, MD 20742, USA

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G1!'+4F$$B!East-West Center for Space Science, University of Maryland, College Park, MD 20742, USA

!

21!%#>$F5!(121!(#3045!D1S1!8/>5!&191!<$$5!9121!N+-;5!L191!'#/05!C1!')05!8191!'3045!S1!"+:0$$>!CHEP, Kyungpook National University, 702-701 Daegu, South Korea

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%1%1&1!C$*/*5!%1!N+3E5!D1!B+0!C)0;5!L1!B+0!W:5!%1%1!9)$-/04!National Aerospace Laboratory, NLR, NL-1 8300 AD Emmeloord, The Netherlands

!

D1!(+:.$**/0/TU5VU!CNR-IROE, I-50125 Florence, Italy

TU!XS6S5!'$A/)0$!F/!J)*)40+5!VU!XS%65(SG5!6/-$0A$!!

L1!"-=>7$-!Max-Planck Institut für extraterrestrische Physik, D-85740 Garching, Germany

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N#1!%AA+-$**)5!N#1!J)3B/$-5!&1!J)3-]3/05!W1!()-./0+5!C1!2++:5!21!2+;),?+05!(1!<$*3@5!'1!S+.+*$5!&1!N+0/@@/+5!W1!N$--/05!&1!N)#*5!C1!G+7/05!(1&1!"/045!&1!9/**$0,-)@;!

DPNC, Université de Genevè, CH-1211 Genevè 4, Switzerland !

'1!J-$)0!NASA Goddard Space Flight Center, GSFC, Greenbelt, MD 20771, USA

!

J1!J+-$.5!%1!J+--+35!D1!J)3F)3*5!&1!J3^0$-F5!<1!C$-)>$5!81!N-).+:)B5!&1!K+-4+:I"-$B/0)5!Z1!K^A/+0.!Laboratoire de Physique Subatomique et de Cosmologie, LPSC, IN2P3/CNRS and Université J. Fourier,

F-38026 Grenoble, France !

8121!D3)5!R121!2$5!O121!23+045!Q121!L/+045!"1Q1!</!5!'1'1!<35!L1P1!S/5!Q1&1!P/5!'1L1!O35!S1'1!Q3!Sun Yat-sen University, Guangzhou, 510275, China

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(1IG1!(#$05!(1!2:/+)5!<1(1!<$$5!L1IG1!":+/!National Space Program Office, NSPO, Hsin-Chu, Taiwan 300

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<1!(#$045!R1D1!D3)5!81!</5!"1!<3+05!<1P1!9+04!Shandong University, Jinan, Shandong, 250100, China

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91!F$!J)$-5!61!2+3*$-5!<1!L304$->+005!(1!'+0F$-5!&1!'@#>+0+35!K1!R#3;)B!IEKP, University of Karlsruhe, D-76128 Karlsruhe, Germany

%1!&3_30$05!L1!G/.+;+-/!Metsahovi Radio Observatory, Helsinki University of Technology, FIN-02540 Kylmala, Finland

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61!J+-+)TU5VU5!D1!J+--$/-+TU5!&1!N/>$0.+TU5VU5!N1!D)0@+*B$:TU5!<1!%--3F+TU5!G1!N$-$/-+TU!Laboratorio de Instrumentacao e Fisica Experimental de Particulas, LIP, P-1000 Lisboa, Portugal

TU LIP, Av. Elias Garcia, 14 1-andar 1000 Lisboa, VU IST, Av. Rovisco Pais, 1049 Lisboa

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O1IL1!6+0@#/+045!21!L/0@#/5!O1I"1!"/04!Chung-Shan Institute of Science and Technology, CSIST, Lung-Tan, Tao Yuan 325, Taiwan

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&1!%43/*+-IJ$0`.$A5!L1!%*@+-+A5!L1!J$-F34)5!L1!(+:+3:5!L1!C$!K/@$0.$5!(1!C`+A5!<1!D+-@`+I"+,+-^:5!W1!<+0@/)../5!D1!&+-.`0$A5!(1!N+*)>+-$:5!(1!&+a+5!L1!&+-`05!&1!&)**+5!W1!'+0@#$A5!'1!'+0A5!X1!'$B/**+5!

61!")-+*5!%1!")--$0.)5!(1!K+A]3$A!Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, CIEMAT, E-28040 Madrid, Spain

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%1!&$0@#+@+!G)@#+!Instituto de Fisica, Universidad Nacional Autónoma de México, UNAM, Mexico D. F., 01000 Mexico

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D1!J)$**+TU5VU5!&1!L1!J):@#/0/TU5VU5!&1!D$-B+:/TU5VU5!C1!D-+0F/TU5VU5!C1!N$F-/0/TU5VU5!'1!N$0:)../!TU5VU5!N1D1!G+0@)/.+TU5!<1!G)::/!TU5!D1!K)*7/0/TU5VU!

University of Milano-Bicocca and INFN-Sezione di Milano, I-20133 Milan, Italy TU!INFN-Sezione di Milano,!

VU!Universita’ di Milano

!

L1!J)*>)0.5!%1!L+@#)*;)E:;+5!&1!'+7/0:;/5!(1!R3-,+@#!Groupe d'Astroparticules de Montpellier, GAM, IN2P3/CNRS-Universite Montpellier II, F-34095 Montpellier,

France !

W1!(#3>/*)B5!O31!D+*+;./)0)B5!K1!N*?+:;/05!%1!'3B)-)B!Institute of Theoretical and Experimental Physics, ITEP, Moscow, 117259 Russia

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X1!&/.-)H+0)B!Institute for Space Research, IKI, Russian Academy of Sciences, Moscow, 117810 Russia

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%1!D-$@#;)5!'1!K):.-/;)B5!S1!(#$-0)7*$;)B!Kurchatov Institute, Moscow, 123182 Russia

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D1!J+:#/0FA#+4?+05!&1!&$-;/05!&1!N+0+:?3;!Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, 119992, Russia

!

L1!D)045!D1P1!D35!L1P1!</!5!P1!</!5!L1R1!<3)5!P1!&$045!<1D1!'#3+/5!21!O/5!(1G1!R)3!Southeast University, Nanjing 210096, China

!

%1!(#/;+0/+05!W1!6/0@#5!G1!&+_;+5!L1!'+0FE$/::!Physics Department, Yale University, New Haven, CT 06520, USA

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J1!%*7+.TU5!D1!%>,-):/TU5!%1!C+>/+>)VU5!%1!N/*3:)VU5!G1!J+../:.)0TU5VU5!J1!J$-.3@@/TU5VU5!'1!J/AA+4*/+TU5!'1!J*+:;)TU5VU5!91L1!J3-4$-TU5!C1!(+-+HH/0/TU5VU5!(1!($@@#/TU5VU5!D1!W:7):/.)TU5VU5!W1!6/+0F-/0/!TU5VU5!W1!6/)-/TU5VU5!D1!<+>+00+YU5!&1!&$0/@#$**/TU5!&1!N+3*3AA/TU5VU5!N1!R3@@)0TU5!%1!N+7/TU5!&1!J/AA+--/TU5VU5!<1!C/!&+:::)TU5VU5!

D1!'@)*/$-/TU5!'1!P/3[U!INFN-Sezione di Perugia and Universitá Degli Studi di Perugia, I-06100 Perugia, Italy

TU!INFN, Sezione di Perugia, VU!Universita’ di Perugia,

YU!Present address CPPM, Marseille, France, [U!Present address China

!

61!($-B$**/TU5!'.1!C/!6+*@)TU5VU5!'.1!D+*$)../TU5!61!D#$-+-F3@@/TU5!&1!X0@+4*/TU5!"1!<)>.+FA$TU5!(1!&+4+AAbTU5!%1!Z-:/0/TU5!W1!N$F-$:@#/TU5!&1!N/$0F/,$0$TU5!61!N/*)TU5VU5!61!'7/0$**+TU5VU5!(1!K+00/0/TU!

INFN-Sezione di Pisa and Universitá di Pisa, I-56100 Pisa, Italy TU!INFN-Sezione di Pisa,

VU!Universita’ di Pisa

!

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61!J-+@@/+H$--/!5!&1!()0.$5!'1!C/!N/77)!Agenzia Spaziale Italiana, ASI, I-00198 Roma, Italy

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%1!%40$0/YU5[U5!'.1!J+@@+-)TU5[U5!%1!J+-.)*)0/!TU5VU5!J1!J)-4/+TU5VU5!(1!J):/)TU5VU5!(1!D+-4/3*)TU5VU5!'1!D$0./*$TU5VU5!&1!&)0.$@@#/TU5[U5!%1!N+)*)AA/TU5YU5!N1!G+7+40+0/TU5VU5!W1!K+*$0.$TU!

INFN-Sezione di Roma and Universitá di Roma “La Sapienza”, I-00185 Roma, Italy TU!INFN, Sezione di Roma,!VU!Universita’ di Roma,!YU!Dip. Ingegneria Aerospaziale, Roma,![U!ENEA, Roma

!

L1!O+045!81!8/>!Ewha Womens University, 120-750 Seoul, South Korea

!

91L1!C/045!%1R1!D35!R1L1!L/05!91'1!</05!P1L1!N+045!91Q1!P/+)5!L121!'#/5!O1&1!'#/5!G1'1!9+045!'191!Q/$5!P121!O$!

Shanghai Jiaotong University, SJTU, Shanghai 200030, China !

W1!6+*@#/0/TU5VU5!N1!&+$:.-)TU5VU5!N1'1!&+--)@@#$:/TU5VU!INFN-Sezione di Siena and Universita’ di Siena, I- 53100 Siena

TU!INFN-Sezione di Siena, VU!\0/B$-:/.+c!F/!'/$0+!!

(1W1!</05!O1I(1!(#+)!Dept. of Aeronautics and Astronautics, National Cheng Kung University, NCKU, Tainan, 701 Taiwan

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'1(1!<$$5!O1!<$/5!R1!G$05!(1!9+05!O1!R#)3!Institute of Physics, Academia Sinica, Taipei 11529, Taiwan

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G121!ZdS$+*5!L-1!AstroParticle and Cosmic Radiation Detector Research and Development Laboratory, Florida A&M University,

Tallahassee, FL 32307, USA !

G1L1!D+-@/+!<)7$A5!(1!C$*4+F)!Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain

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%1!&)0H+-F/0/5!N1!"-+>73:!Center for Adanced Research in Space Optics, CARSO, 34012 Trieste, Italy

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"1!W-)0$05!"1!<+/./0$05!W1!G//#)0$05!L1!")-:./5!W1!K+*.)0$0!University of Turku, FIN-20014 Turku, Finland

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21!%0F$-#3,5!%1!J/*+0F5!21!2)H$-5!61!N+3::5!L1!\*,-/@#.5!D1!K/$-.$*!Eidgenössische Technische Hochschule, ETH Zürich, CH-8093 Zürich, Switzerland

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Contents!

Introduction: The Alpha Magnetic Spectrometer (AMS) !!!T!

Chapter One: AMS-01, engineering flight on the Space Shuttle TIT!

T1T! ()0:.-3@./)0!)H!.#$!%&'IeT!&+40$.! TIT!

T1V! %&'IeT!'/*/@)0!"-+@;$-! TI[!

T1Y! %&'IeT!()30.$-!'?:.$>:! TIf!

T1[! %&'IeT!W*[email protected])0/@:! TIg!

T1h! %&'IeT!Z7$-+./)0:! TITT!

T1i! %&'IeT!N#?:/@:! TITY!

Chapter Two: AMS-02, particle physics on the International Space VIT!

V1T! (-?)>+40$.! VIV!

V1V! "-+0:/./)0!G+F/+./)0!C$.$@.)-!j"GCU! VIVg!

V1Y! '/*/@)0!"-+@;$-! VIh[!

V1[! "/>$!)H!6*/4#.!j"Z6U! VIkT!

V1h! %0./@)/0@/F$0@$!()30.$-:!j%((U! VIgk!

V1i! G/04!X>+4/04!($-$0;)B!C$.$@.)-!jGX(2U! VITeV!

V1f! W*[email protected])>+40$./@!(+*)-/>$.$-! VITTi!

V1k! W*[email protected])0/@:! VITYi!

V1g! "#$->+*!()0.-)*! VITik!

V1Te! X0.$4-+./)0! VITff!

V1TT! Z7$-+./)0:! VITge!

V1TV! %&'IeV!N#?:/@:!WM+>7*$:! VITgY!

Conclusion and Acknowledgements! !

Appendices! !

%! %,,-$B/+./)0!+0F!%@-)0?>:! !

J! %&'!7-/0@/7+*!73,*/@+./)0:! !

(! ()**+,)-+./04!X0:./.3./)0:!+0F!\0/B$-:/./$:! !

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Introduction: The Alpha Magnetic Spectrometer (AMS)

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Page 10: 2004 Ams Nim Paper Draft

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Mexico

56 Universities, 498 Physicists56 Universities, 498 Physicists

NASA provides: Three shuttle flights with Mission Management at JSCNASA provides: Three shuttle flights with Mission Management at JSCAMS is an International Experiment

CHINA

RUSSIAFINLAND

GERMANY

DENMARKEUROPE ASIAUSA

USA

NETHERLANDS

ITALY

MEXICO

BISEECALTIEEIHEPSJTUSEUSYSUSDUAcademia SinicaCSISTNCUNCKUNCTUNSPO

(Taiwan)

(Beijing)(Beijing)(Beijing)(Beijing)(Shanghai)(Nanjing)(Guangzhou)(Jinan)

(Taiwan)(Chung Li)(Tainan)(Hsinchu)(Hsinchu)

KOREAEWHAKYUNPOOK NAT. UNIV.

MOSCOW STATE UNIV.KURCHATOV INST.ITEPI.K.I.

PORTUGALLAB. OF INSTRUM. LISBON

SPAINCIEMAT - MADRIDI.A.C. , CANARIAS

SWITZERLANDETH-ZurichUNIV. OF GENEVA

ROMANIAUNIV. OF BUCHAREST

ESTECNLRNIKHEF

UNIV. OF AARHUS

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CARSO TriesteIROE FlorenceINFN and UNIV. OF BOLOGNAINFN and UNIV. OF MILANOINFN and UNIV. OF PERUGIAINFN and UNIV. OF PISAINFN and UNIV. OF ROMAINFN and UNIV. OF SIENA

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Portugal

Spain

France

NetherlandsDenmark

Finland

Germany

Switzerland

Italy

Russia

China

Taiwan

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Figure 1: Participation in AMS from the U.S.A., Europe and Asia.

Page 11: 2004 Ams Nim Paper Draft

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Figure 2: A TeV Detector in Space: AMS-02 on the Space Station. "#$!B+*3$!)H!sPs!/:!>$+:3-$F!/0F$7$0F$0.*?!/0!"-+@;$-5!GX(2!+0F!"Z61!"#$!:/40$F!@#+-4$5!tP5!+0F!.#$!>)>$0.3>!)H!.#$!7+-./@*$5!N5!+-$!>$+:3-$F!,?!.#$!k!*+?$-:!)H!F)3,*$FI:/F$F!:/*/@)0!.-+@;$-!/0!.#$!>+40$.1!

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Page 12: 2004 Ams Nim Paper Draft

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Figure 3: Rigidity Resolution of protons and He in AMS-02. !

Page 13: 2004 Ams Nim Paper Draft

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References

mTn! L1!W**/:!et al.5!N#?:1!<$..1!B214 jTggkU!Yp!&1!"3-0$-!+0F!61!9/*@A$;5!N#?:1!G$B1!D42!jTggeU![p!W1%1!J+*.A!+0F!L1!WF:_)5!!N#?:1!G$B1!D59!jTgggU!VYhTTp!"1!&)-)/!+0F!<1!G+0F+**5!S3@1!N#?:1!B570!jVeeeU![hh1!

mVn! N1!'+*+./5!et al.5!S3@*1N#?:1N-)@1'377*1!81!jVeeeU!Yf1!

mYn! &1!G?*$!+0F!%12$B/:#5!S),$*!6)30F+./)0!C/-$@.)-?!jVeeYU1!

m[n! N1<1!8+7/:.+5!%1N$0A/+:!+0F!G191!9/*:)05!S),$*!6)30F+./)0!C/-$@.)-?!jVeeYU1!

mhn! G1%1!23*:$!+0F!L1!"+?*)-5!S),$*!6)30F+./)0!C/-$@.)-?!jVeeYU1!

"#$!$M7$-/>$0.:!0).$F!#+B$!73,*/:#$F!>+0?!B+*3+,*$!7+7$-:5!E#/@#!+-$!*/:.$F!+.!.#$!0).$F!\G<:l!

min! #..7luu#$+:+-@14:H@10+:+14)BuF)@:u-):+.u-):4)H1#.>*!

mfn! #..7luu#$+:+-@14:H@10+:+14)BuF)@:u@):,u@):,1#.>*!

mkn! #..7luu*+>,F+14:H@10+:+14)Bu7-)[email protected]@),$u!

mgn! #..7luu#$+:+-@14:H@10+:+14)BuF)@:u@4-)u@4-)1#.>*!

mTen! #..7luu#$+:+-@14:H@10+:+14)BuF)@:u+:@+u+:@+4)H1#.>*!

mTTn! #..7luu#$+:+-@14:H@10+:+14)BuF)@:uM.$uM.$xT:.1#.>*!

mTVn! #..7luu#3,,*$10+:+14)Bu!

mTYn! #..7luu*#$+EEE14:H@10+:+14)BuF)@:u4+>@):-+?u#$@-uJW''uJW''1#.>*p!21!&+.:30+4+!et al.5!N#?:1!G$B1!<$..1!81!jTggkU![ehVp!%1!&)/:$$B!et al.5!%:.-)7#?:/@+*!L)3-0+*!474!jTggfU![kgp!'1!Z-/.)!et al.5!N-)@$$F/04:!)H!X(2WN5!K+0@)3B$-!jTggkUp!L161!Z->$:!et al.5!%71!L1!<$..1!482!jTggfU!<Tkfp!"1!'+$;/!et al.5!N#?:1!<$..1!B422!jTggkU!YTgp!W1'1!'$)!et al.5!Vh.#!X(G(!5!jTggfU!YfYp!%1!O+>+>).)!et al.5!%FB+0@$:!/0!'7+@$!G$:$+-@#!14!jVU!jTgghU!fhp!81!O):#/>3-+!et al.5!N#?:1!G$B1!<$..1!75!jTggiU!YfgV1!

Page 14: 2004 Ams Nim Paper Draft

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mThn! J+-E/@;!et al15!SX&!400!jTggfU!Y[1!

mTin! #..7luu/F+T17#?:/;130/I:/$4$01F$u@+7-/@$1#.>*p!&1!J)$A/)!et al.,!%71!L1!532!jVeeeU!ihYp!&1!J)$A/)!et al.,!N#?:1!G$B1!D62!jVeeeU!eYVeef!L1!8-$>$-!et al.,!N#?:1!G$B1!<$..1!83,!y!VT!jTgggU![V[Tp!&1!J)$A/)!et al.,!N#?:1!G$B1!<$..1!82,!y!V[!jTgggU![fhfp!"1!6-+0@;$!et al.,!Vi.#!X(G(!2!jTgggU!kep!&1!J)$A/)!et al.,!%71!L1!518!jTgggU![hf!D1!J+-,/$**/0/!et al.,!Vh.#!X(G(!6!jTggfU!YTfp!D1!J+-,/$**/0/!et al.,!Vh.#!X(G(!3!jTggfU!Yigp!D1!J+-,/$**/0/!et al.,!Vh.#!X(G(!4!jTggfU!VTfp!D1!J+-,/$**/0/!et al.,!Vh.#!X(G(!4!jTggfU!VVTp!D1!J+-,/$**/0/!et al.,!Vh.#!X(G(!3!jTggfU!Yffp!&1!J)$A/)!et al.,!%N1!L1!487 jTggfU![Thp!D1!J+-,/$**/0/!et al.,!%z%!309!jTggiU!<Thp!D1!J+-,/$**/0/!et al.,!S3@*1!X0:.-1!&$.#1!A371!jTggiU!Tigp!&1!J)@@/)*/0/!et al.,!S3@*1!X0:.-1!&$.#1!A370!jTggiU![eYp!D1!J+-,/$**/0/!et al.,!V[.#!X(G(!3!jTgghU!kep!D1!J+-,/$**/0/!et al.,!V[.#!X(G(!3!jTgghU!ihfp!N1!(+-*:)0!et al.,!S3@*1!X0:.-1!&$.#1!A349!jTgg[U!hffp!N1!(+-*:)0!et al.,!VY-F!X(G(!2!jTggYU!he[1!

mTfn! #..7luu/F+T17#?:/;130/I:/$4$01F$u&+::V1#.>*p!(1!D-/>+0/!et al.,!%z%!392!jVeeVU!Vkfp!&1!(/-@$**+!et al.,!Vi.#!X(G(!jTgggU!'21Y1i1Tkp!D1!J+:/0/!et al.,!Vi.#!X(G(!jTgggU!ZD1T1T1VTp!G1!J$**)../!et al.,!N#?:1!G$B1!C!60!jTgggU!ehVeeVp!&1!(/-@$**+!et al.,!Vh.#!X(G(!6!jTggfU!YkTp!&1!2)H!et al.,!%71!L1!467!jTggiU!<YYp!D1J+:/0/!et al.,!V[.#!X(G(!3!jTgghU!Tp!(1D-/>+0/!et al.,!V[.#!X(G(!4!jTgghU!TeVgp!D1J+:/0/!et al.,!V[.#!X(G(!1!jTgghU!hkhp!N1N+7/0/!et al.,!V[.#!X(G(!4!jTgghU!TeYYp!&1!2)H!et al.,!V[.#!X(G(!3!jTgghU!iep!D1!J+:/0/!et al.,!VY-F!X(G(!3!jTggYU!ffY1!

mTkn! #..7luuH*+@)10>:31$F3p!&1!2)H!et al.,!%71!L1!467!jTggiU!YY1!

mTgn! C1W**/.#)-7$5!N#C!"#$:/:5!\1!)H!(#/@+4)!jTggkU1!

mVen! #..7luu#$+:+-@14:H@10+:+14)BuF)@:u#$+)Yu#$+)Y1#.>*p!91%1!&+#)0$?!et al.,!S3@*1!X0:.-1!&$.#1!178!jTgkeU!YiY1!

mVTn! #..7luuEEE1:;?-)@;$.1F$u:7+@$uF)@x:F+.u+-/$*Ih1#.>p!81%1!N)30F:5!G%'!P3+-.$-*?!27!jTgkiU![Yh1!N121!6)E*$-!et al.,!Tf.#!X(G(!jTgkYU!

mVVn! #..7luuEEE1:-*1@+*.$@#1$F3u%(Wup!'7+@$!'@/$0@$!G$B/$E:!86!jTggkU!Tu[1!

!

Page 15: 2004 Ams Nim Paper Draft

! f

mVYn! #..7luu*#$+EEE14:H@10+:+14)BuF)@:u4+>@):-+?u*$@-uWN%("[email protected]#.>*p!C1K1!G$+>$:!$.!+*15!%FB1!'7+@$!G$:1!19.5!jTggfU!keg1!

mV[n! #..7luu#$*/)1$:.$@1$:+10*u3*?::$:up!C1C1!J+-,):+!+0F!&1D1!8/B$*:)05!'@/$0@$!257!jTggVU!T[kf1!!

mVhn! #..7luuB)?+4$-1_7*10+:+14)Bu/0F$M1#.>*p!#..7luuB)?+4$-1_7*10+:+14)Bu:@/$0@$u,/,*/)4-+7#?x@-:1#.>*1!

mVin! N121!6)E*$-!et al.,!%:.-)1!N+-.1!N#?:1!15!jVeeTU![g1!

mVfn! #..7luuEEE1+34$-1)-4up!#..7luuEEE1+34$-1)-4u+F>/0uC$:/40G$7)-.u/0F$M1#.>*1!

mVkn! (1!C$!&+-A)!$.!+*15!S3)B)!(/>$0.)!9C!jTgkiU!VkT1!

mVgn! Z*/B$-!et al.,!S3@*1!X0:.-1!&$.#1!A276 jTgkgU!YfT1!

mYen! #..7luuEEEI:;1/@--13I.);?)1+@1_7uF)@u:;p!"#$!'37$-I8+>/);+0F$!()**+,)-+./)05!N#?:1!G$B1!<$..1!81!jTggkU!ThiV1!

mYTn! L1D1!%:,3-?!et al.,!N#?:1!G$B1!<$..1!185!V!jTgifU!ihp!! L1D1!%:,3-?!et al.,!N#?:1!G$B1!<$..1!195!Th!jTgifU!kigp!! \1!J$@;$-!et al.,!N#?:1!G$B1!<$..1!215!VT!jTgikU!The[p!! 21!%*B$0:*$,$0!et al.,!N#?:1!G$B1!<$..1!275!TY!jTgfTU!kkk1!

mYVn! L1L1!%3,$-.!et al.,!N#?:1!G$B1!<$..1!335!VY!jTgf[U!T[e[1!

mYYn! 6)-!$M+>7*$5!<Y!()**+,)-+./)05!S3@*1!X0:.-1!&$.#1!%!289!jTggeU!Yh1!

mY[n! G1J+../:.)0!et al.5!%:.-)1!N+-.1!N#?:1!13!jVeeeU!hT1!

Page 16: 2004 Ams Nim Paper Draft

!k!

!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !

AM

S

Fig

ure 4

: View

of A

MS

on

the IS

S.

Page 17: 2004 Ams Nim Paper Draft

! "#"

Chapter One: AMS-01, engineering flight on the Space Shuttle

$%&'(%! )*+,-..-,)'*! '*! ,/%! 01-2%! 0,-,)'*3! 450! 1%(&'(6%7! -*! %*8)*%%()*8! &.)8/,! '*! ,/%! 01-2%!

0/9,,.%!,'!%*+9(%!,/-,:!!!

+ ;/%!450!%<1%()6%*,!2-*!&9*2,)'*!1('1%(.=!)*!+1-2%>!)*!?-2996!@),/!'(A),-.!,%61%(-,9(%!2/-*8%+!

&('6!!BC!,'!DE!,F!-*7!)*!,/%!)*,%*+%!(-7)-,)'*!A-2G8('9*7!H@/)2/!2'*,-)*+!/%-?=!*92.%)!2-9+)*8!+)*8.%!%?%*,!.-,2/#91!)*!2/)1+IJ!!

+ ;/%!7%,%2,'(!2-*!@),/+,-*7! ,/%! ,(%6%*7'9+!?)A(-,)'*+!H"CE!7$I!-*7!-22%.%(-,)'*!HK!8I!-,! .-9*2/!-*7!,/%!7%-22%.%(-,)'*!HBJC!8I!-,!.-*7)*8>!

;/)+! 6)++)'*! @-+! +9A+%L9%*,.=! (%&%((%7! ,'! -+! 450#E"J! ! ;/%! %<1%()6%*,-.! 2'*&)89(-,)'*! )+! +/'@*! )*!M)89(%!"J"J!

!

Honeycomb

Silicon Wafers

Honeycomb

Computers

Time of FlightCounters

Aerogel

Magnet

Electronics

Foam

Time of FlightCounters

Low Energy Particle Shield

Veto

Cou

nter

s

!

Figure 1.1: AMS-01, the configuration for the Space Shuttle flight.

1.1 Construction of the AMS-01 magnet!;/%!450#E"!6-8*%,!@-+!6-7%!&('6!BD!/)8/#8(-7%!N7#M%#$!+%2,'(+J!!O-2/!+%2,'(!@-+!2'61'+%7!

'&!"EE!HPQ!<!PQ!<!"QI!A.'2G+J!!M)89(%!"JP!+/'@+!,/%!-((-*8%6%*,!'&!,/%!&)%.7!7)(%2,)'*!'&!,/%!BD!+%2,'(+J!!;/%!/)8/%+,!8(-7%!N7#M%#$!A.'2G+3!@),/!-*!%*%(8=! .%?%.!'&! H$RI6-<!S!CE!<!"E

B!TU%3!@%(%!9+%7J! !;/)+!

Page 18: 2004 Ams Nim Paper Draft

AMS-01/Magnet

!"#P!

2'*&)89(-,)'*!1('792%7!-!7)1'.%! &)%.7!'&!"JC!GT!-*7!-!*%8.)8)A.%!7)1'.%!6'6%*,"J! ! V*!-77),)'*3! ,/%!&.9<!.%-G-8%P!-,!-!P#6%,%(!7)+,-*2%!&('6!,/%!2%*,%(!'&!,/%!6-8*%,!)+!K!TJ!!!

Permanent Magnet(with high grade Nd-Fe-B)

B (Earth) ! 0.5 G

The Magnetic Dipole Moment = 0

1 2 3 4 56

78

910

1112

1314

1516

"""" " " " "

""

""

""

""

""

""

""

"

""

""

"""""""

"""

""

""

""

"" " " " "

"""""

""

""

""

""""

B!1.5KG1.5KG

X

Y

!1 ML !1 M#

!!

Figure 1.2: Magnetic field orientation of the AMS-01 magnet.

$%&'(%! ,/%! 2'*+,(92,)'*!'&! ,/%! &9..! +2-.%!6-8*%,+3! -! ":K! +2-.%!6-8*%,!@-+!A9).,! ,'! 2'*&)(6!-*7!6%-+9(%! ,/%! &)%.7! )*+)7%! ,/%! 6-8*%,3! ,/%! 7)1'.%! 6'6%*,! -*7! ,/%! &.9<! .%-G-8%J! ! ;/%*! ,/(%%! &9..! +2-.%!6-8*%,+!@%(%!A9).,:!!

H)I! ,/%!&)(+,!6-8*%,!@-+!9+%7!)*!-22%.%(-,)'*!-*7!?)A(-,)'*!,%+,+!&'(!+1-2%!L9-.)&)2-,)'*>!

H))I! ,/%!+%2'*7!6-8*%,!@-+!,/%!&.)8/,!6-8*%,>!

H)))I! ,/%!,/)(7!6-8*%,!@-+!A9).,!@),/'9,!8.9%!&'(!N404!+-&%,=!,%+,+J!

M)89(%!"JK!+/'@+!,/%!7)6%*+)'*+!'&!,/%!450#E"!&.)8/,!6-8*%,J!!4+!+/'@*!)*!M)89(%+!"JD!-*7!"JC3!,/%+%!6-8*%,+!@%(%!+9AW%2,%7!,'!-!&9..!A-,,%(=!'&!+1-2%!L9-.)&)2-,)'*!,%+,)*8J!!!

;/%!,/)(7!&9..!+2-.%!6-8*%,!@-+!A9).,!A%2-9+%!'&!,/%!.-2G!'&!G*'@.%78%!'&!,/%!8.9%!1%(&'(6-*2%!'?%(!-*!%<,%*7%7!1%()'7!'&!,)6%!)*!,/%!+1-2%!%*?)('*6%*,J!!V,!@-+!A9).,!@),/'9,!9+)*8!-*=!8.9%!,'!A%!,%+,%7!,'!7%+,(92,)'*!,'!%*+9(%!,/-,!450!2'9.7!A%!(%,9(*%7!'*!,/%!0/9,,.%!,'!O-(,/!%?%*!)&!,/%!8.9%!2'61.%,%.=!&-).%7!@/).%!'*!'(A),J!!!

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!"!! ;/%!8%'6-8*%,)2!&)%.7!)+!EJC!T!'*!,/%!+9(&-2%!-*7!?-()%+!@/%*!'*!'(A),J!!4!+,('*8!7)1'.%!6'6%*,!@'9.7!(%+9.,!)*!-*!

9*7%+)(-A.%!&'(2%!'*!,/%!+1-2%!+/9,,.%!'(!,/%!+1-2%!+,-,)'*J!P!! N404!(%L9)(%+!,/%!.%-G-8%!&)%.7!,'!A%!X!KEET!+'!-+!*',!,'!)*,%(&%(%!@),/!,/%!.)&%!+911'(,!+=+,%6!'&!,/%!-+,('*-9,+J!

Page 19: 2004 Ams Nim Paper Draft

AMS-01/Magnet

! "#K

Innershell

OuterShell

Nd-Fe-B

x

y

z

0

86.5

1115

3

800

1299

Acceptance = 0.82 m2srBL2 = 0.15 TM2

Weight = 1900 kg

Bx=1.5 KG

!!

Figure 1.3: Properties of the AMS-01 flight magnet. !

!!

Figure 1.4: AMS-01 magnet during vibration tests at the Beijing Institute

of Spacecraft Environment and Engineering in Beijing, China.

Page 20: 2004 Ams Nim Paper Draft

AMS-01/Magnet

!"#D!

!

Figure 1.4: AMS-01 magnet undergoing centrifuge (static load) testing

at the Laboratory for Centrifugal Modeling in Beijing, China.

1.2 AMS-01 Silicon Tracker M)89(%!"JB!+/'@+!,/%!.'2-,)'*!'&!,/%!+)<!1.-*%+!'&!,/%!0).)2'*!;(-2G%(!H;"#;BI!)*!450#E"J!!!

!Particle trajectory

B = 0.14T

Perm

an

en

t M

ag

net

Nd

-Fe-B

: 4

6 M

GO

e

AC

C

AC

C

1 m

AerogelCerenkov

TOF Layers

LEPS

S2

yz

x

T1T2

T3

T4

T5T6

TrackerPlanes

S3

S4

S1 !

"

#

$

%

!!

Figure 1.6: Location of the Silicon Tracker in AMS-01. M'(!,/)+!%*8)*%%()*8!&.)8/,!K!'&!,/%!B!6P!'&!+).)2'*!@%(%!)*+,-..%73!-+!+/'@*!)*!(%7J!

!

Page 21: 2004 Ams Nim Paper Draft

AMS-01/Tracker

! "#C

;/%! 7%+)8*! -*7! 2'*+,(92,)'*! '&! ,/%! ;(-2G%(! A%*%&),%7! &('6! ,/%! 2'*+,(92,)'*! -*7! '1%(-,)'*-.!%<1%()%*2%!'&! ,/%!0).)2'*!5)2('?%(,%<!Y%,%2,'(! H05YI!-,! ,/%!ZK!%<1%()6%*,J! !M'(! ,/%!450#E"! +/9,,.%!&.)8/,3!K!6P!'&!7'9A.%#+)7%7!+).)2'*!+%*+'(+!@%(%! )61.%6%*,%73!-! ,',-.!'&![E3EEE!(%-7'9,!2/-**%.+J! !;/%!

(%+'.9,)'*!@-+!"E!-6#)*!,/%!A%*7)*8!1.-*%!-*7!KE!-6!)*!,/%!*'*#A%*7)*8!1.-*%3!'(!.\]\!S![^!-,!"E!T%_J!!!

;/%! +).)2'*! .-77%(+! @%(%! @(-11%7! )*! -*! 9.,(-#,/)*! 2'11%(! 2'-,%7! %.%2,('6-8*%,)2! +/)%.7J! ! ;/%!.-77%(+! @%*,! ,/('98/! %.%2,('6-8*%,)2! HO5I! 2'61-,)A).),=! ,%+,+! )*! ,/%! GR`3! 5R`! -*7! TR`! (-*8%+! ,'!%+,-A.)+/!O5!)669*),=!.%?%.+J!!;/%!2'61.%,%7!.-77%(+!@%(%!-++%6A.%7!'*!+)<!,/)*!/'*%=2'6A!1.-,%+!@),/!-! 2'6A)*%7! ,/)2G*%++3! )*! (-7)-,)'*! .%*8,/+3! '&! a]aE! X! KJP^J! ! O-2/! 1.-,%3!6%-+9()*8! "!6! )*! 7)-6%,%(3!2'*,-)*%7! 1(%2)+)'*! /'.%+! &'(! -,,-2/)*8! ,/%! +).)2'*! .-77%(+! -*7! %*+9()*8! ,/%)(! &.-,*%++! ,'! bE!-6J! !;/%=!@%(%!7%+)8*%7!,'!-..'@!,/%!.-77%(+!,'!A%!-.)8*%7!)*7%1%*7%*,.=!'&!,%61%(-,9(%3!/96)7),=!-*7!-)(!1(%++9(%!2/-*8%+J!!!

M)89(%!"J[! +/'@+! ,/%! )*,%8(-,)'*! '&! ,/%! +).)2'*! .-77%(+! '*! '*%! '&! ,/%! +)<! 1.-,%+J! ;/%! +911'(,!+,(92,9(%!&'(!,/%!+)<!1.-*%+3!-.+'!+/'@*!)*!M)89(%!"Jb3!@-+!6-7%!&('6!-!2-(A'*!2'61'+),%!6-,%()-.!,'!A%!.)8/,#,)8/,! -*7! %L9)11%7!@),/! -! 2''.)*8! +=+,%6! ,/-,! (%6'?%+! /%-,! 1('792%7! A=! ,/%! ,(-2G%(c+! &('*,#%*7!%.%2,('*)2+J!!!!

! !! !!

Figure 1.7: Integration of silicon ladders on one of six ultralight plates (left). Final

preassembled silicon tracker carbon-fiber composite (CFC) mechanical

structure including the CFC upper and lower support flanges (right). !

;'!%*+9(%!,/-,!,/%!450#E"!7%,%2,'(!/-7!,/%!7%+)(%7!-229(-2=3!-*!)*&(-(%7!.-+%(!-.)8*6%*,!+=+,%6!@-+! 7%?%.'1%7J! ! ;/%! .-+%(! A%-6+! 1-(,)-..=! )'*)`%! ,/%! +).)2'*! -+! ,/%=! ,(-?%(+%! ,/%!;(-2G%(! 1.-*%+J! ! ;/%!+=+,%6!1('?)7%+!1'+),)'*-.!-229(-2=!'&!-!1-++)*8!1-(,)2.%!,/('98/!%-2/!'&!,/%!+)<!1.-*%+!,'!@),/)*!-!&%@!6)2('*+J!;/)+!+=+,%6!)+!+/'@*!)*!M)89(%!"JbJ!!!

!

Page 22: 2004 Ams Nim Paper Draft

AMS-01/Tracker

!"#B!

Honeycomb Plane 1

Honeycomb Plane 2

Honeycomb Plane 3

Honeycomb Plane 4

Honeycomb Plane 5

Honeycomb Plane 6

Support Shell

AMS trackerSTS 91 configuration

Beamport Channel

TAS Laser Beams

xAMS

yAMS

Si detectorson ladders

Ladder readout (hybrids)

Support Foot

Inner Thermal Bars

Outer Thermal Bars

Tracker Flange

Thermal ContactSquare Tubes

!

Figure 1.8: Laser alignment system for the AMS-01 Tracker.

;/%!&('*,#%*7!%.%2,('*)2+!'&!,/%!;(-2G%(!@%(%!6-7%!'&!?%(=!.'@!*')+%!_Z0V!9*),+J!!O-2/!2/-**%.!2'*+)+,+!'&!-!+-61.%!-*7!/'.7!.'@#*')+%!2/-(8%!1(%-61.)&)%(J!!;/%=!-(%!(%-7!'9,!+%L9%*,)-..=!-,!+1%%7+!91!,'!C!5R`J!!;/%!7-,-!(%792,)'*!%.%2,('*)2+!&'(!,/%!;(-2G%(!@%(%!+1%2)-..=!7%+)8*%7!,'!A%!.)8/,!@%)8/,!-*7!9+%! 6)*)696! 1'@%(J! ! ;/%! .-77%(+! -*7! -..! ,/%! 7-,-! (%792,)'*! +=+,%6+! @%*,! ,/('98/! ?)8'('9+! +1-2%!L9-.)&)2-,)'*!,%+,)*8!)*2.97)*8!-22%.%(-,)'*3!?)A(-,)'*3!,/%(6-.!?-2996!-*7!,%61%(-,9(%!,'.%(-*2%J!!!

;/%! .-77%(+!@%(%! ,%+,%7! )*!-!/%-?=! )'*! ,%+,!A%-6!-,! ,/%!T%+%..+2/-&,! &d(!02/@%()'*%*&'(+2/9*8!HT0VI!Y-(6+,-7,3!T%(6-*=3!@),/!R3!R%3!Z)!-*7!FJ!!M)89(%!"Je!7%6'*+,(-,%+!,/%!7O]7a!(%+1'*+%!.)*%-(),=!)*!6)*)696!)'*)`)*8!1-(,)2.%!H5V\I!%L9)?-.%*,+J!

!

H

He

Li

B

C

He, Li, B, C carbon beam data

H electron beam data

0

200

400

600

800

1000

1200

1400

1600

1800

2000

5 10 15 20 25 30 35 40

Ch

arg

e (A

DC

ch

an

nels

)

MIP equivalent !!

Figure 1.9: Response of AMS-01 Silicon Ladders.

Page 23: 2004 Ams Nim Paper Draft

AMS-01/Counters

! "#[

1.3 AMS-01 Counters 450#E"!2'*,-)*%7!,/(%%!,=1%+!'&!2'9*,%(+:!_%,'3!;)6%!'&!M.)8/,!-*7!4%('8%.!F%(%*G'?J!

1.3.1 The veto counters

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

!

!!

Figure 1.10: Final flight assembly of the 16 module veto counter system in the AMS-01 magnet

at ETH-Zürich. The carbon fiber reinforcement cylinder is visible inside. !

1.3.2 The AMS-01 Time of Flight hodoscopes

;/%! ;)6%! '&! M.)8/,! 0=+,%6! 1('?)7%+! ,/%! &)(+,#.%?%.! ,()88%(3! 6%-+9(%+! ,/%! ,)6%! '&! &.)8/,! ,'! -*!-229(-2=!'&!f!"EE!1+!-*7!6%-+9(%+!7O]7a!,'!7%,%(6)*%!,/%!-A+'.9,%!2/-(8%!HgIJ!!;/%!&'9(!.-=%(+!'&!;)6%!'&!M.)8/,!F'9*,%(+!H0"#0DI!%-2/!2'*,-)*!"D!+2)*,)..-,'(!/'7'+2'1%+!H1-77.%+IJ!!O-2/!/'7'+2'1%!)+!?)%@%7!A=!,/(%%!1/','69.,)1.)%(+!-,!%-2/!%*73!-+!+/'@*!)*!M)89(%!"J""J!

!

Page 24: 2004 Ams Nim Paper Draft

AMS-01/Counters

!"#b!

Adobe Systems

!

Figure 1.11: Schematic of AMS-01 Time of Flight counter design.

;/%! ;)6%! '&! M.)8/,! %.%6%*,+! 9*7%(@%*,! %<,%*+)?%! 2-.)A(-,)'*! -*7! +1-2%! L9-.)&)2-,)'*! ,%+,+!)*2.97)*8!?)A(-,)'*!-*7!,/%(6-.!?-2996!,%+,+!)*!,/%!V,-.)-*!-%('+1-2%!)*79+,(=J!!;/%!,/%(6-.!?-2996!,%+,+!@%(%! )*,%*7%7! ,'! 2/%2G! -*7! 2'((%2,! -*=! 1',%*,)-.! /-`-(7'9+! %.%2,()2-.! 7)+2/-(8%! )*! +1-2%J! ! M)89(%!"J"P!+/'@+!,/%!;)6%!'&!M.)8/,!2'9*,%(+!)*+,-..%7!)*,'!450#E"J!!

!

!!

Figure 1.12: Mounting of Time of Flight on AMS-01. !

1.3.3 Aerogel Cerenkov Counter

M'(! ,/%! 450#E"! 0/9,,.%! &.)8/,! @%! (%1.-2%7! ,/%! hVFR! -*7! OF4Z! @),/! 4%('8%.! F%(%*G'?!F'9*,%(+! @/)2/! /-7! -! (%&(-2,)?%! )*7%<! *! S! "JEDJ! ! ;/%! 4%('8%.! 2'9*,%(+! @%(%! 6-7%! '9,! '&! ,@'!+91%()61'+%7! .-=%(+! '&! 2%..+! ""! <! ""! 26P3! %-2/! .-=%(! 2'*+)+,)*8! '&! bE! H,'1I! -*7! bb! HA',,'6I! 2%..+! '&!4%('8%.! A.'2G+J! ! ;/%! 2%..! 7%+)8*! )+! +/'@*! )*! M)89(%!"J"KJ! ! O-2/! 2%..!@-+! )*7)?)79-..=! 2'91.%7! ,'! ,@'!1/','69.,)1.)%(!,9A%+!@/)2/!7%,%2,!F%(%*G'?!.)8/,!&('6!%.%2,('*+!H&('6!PJ"!5%_I3!1)'*+!H&('6!CBE!5%_I!-*7!1(','*+!H&('6!DJEC!T%_IJ!!;/)+!)*&'(6-,)'*!%*-A.%7!9+!,'!)7%*,)&=!-*,)1(','*+!91!,'!D T%_J!

!

Discriminators

PMTs

Paddle

Page 25: 2004 Ams Nim Paper Draft

AMS-01/Counters

! "#e

Aerogel 113,5 • 113,5 • 10

Carbon fibre

Teflon3 • 10 ml

PMT

Circuit

Shielding

Shim

!

Figure 1.13: A cell of the Aerogel Counter.

1.4 AMS-01 Electronics ;/%! %.%2,('*)2+! &'(! 450! )+! 7%()?%7! &('6! '9(! %<1%()%*2%! )*! )*+,(96%*,)*8! ,%((%+,()-.! 1-(,)2.%!

1/=+)2+!7%,%2,'(+J!!592/!2-(%!-*7!-,,%*,)'*!-(%!*%2%++-(=!,'!%*+9(%!,/-,!,/%+%!1-(,)2.%!1/=+)2+!%.%2,('*)2+!2-*!A%!9+%7!)*!+1-2%J!!;/%(%!-(%![E3EEE!2/-**%.+!'&!,(-2G%(!+)8*-.+!@/)2/!1('?)7%!-!2''(7)*-,%!-229(-2=!

'&!"E!-6J!!;/%(%!-(%!&'9(!.-=%(+!'&!;)6%!'&!M.)8/,!/'7'+2'1%+!1('?)7)*8!-!,)6%!(%+'.9,)'*!'&!f!"EE!1+J!!$',/!,/%!0).)2'*!;(-2G%(!-*7!;)6%!'&!M.)8/,!2'9*,%(+!-.+'!1('?)7%!)*7%1%*7%*,!7O]7a!6%-+9(%6%*,+!,'!)7%*,)&=! 1-(,)2.%! 2/-(8%J! ! $%2-9+%! '&! 1'@%(! -*7! @%)8/,! (%+,()2,)'*+3! -..! ,/%! %.%2,('*)2+! @%(%! +1%2)-..=!7%+)8*%73!6-*9&-2,9(%7!-*7!+1-2%!L9-.)&)%7!A=!450!)*+,),9,)'*+!-*7!-%('+1-2%!)*79+,()%+!)*!O9('1%!-*7!4+)-J!

M)89(%!"J"D! +/'@+! -*! '?%(?)%@! '&! ,/%! 450#E"! %.%2,('*)2+! 7%+)8*!@/)2/! )+! A-+%7! '*!69.,)1.%!(%79*7-*2)%+!,'!+-&%89-(7!-8-)*+,!,/%!.'++!'&!7-,-!)*!+1-2%J!!;'!+1-2%!L9-.)&=!,/%!%.%2,('*)2+3!,/%!+=+,%6!@%*,! ,/('98/! %<,%*+)?%! ,%+,+! @/)2/! )*2.97%7:! ?)A(-,)'*3! ,%61%(-,9(%3! ,/%(6-.! ?-29963! (-7)-,)'*! -*7!%.%2,('6-8*%,)2! 2'61-,)A).),=J! ! ;/%! (-7)-,)'*! ,%+,+!@%(%! +1%2)-..=! 2-(()%7! '9,! -,!Y9A*-! -*7! ,/%+%! ,%+,+!@%(%!1-(,)29.-(.=!)61'(,-*,!,'!%*+9(%!,/%(%!@'9.7!A%!*'!+)*8.%!%?%*,!.-,2/!91!)*!+1-2%J!!;-A.%!"J"!+/'@+!,/%!A%-6!-*7!%*%(8=!9+%7! )*! ,/%+%! ,%+,+J! !;/%! +1-2%!L9-.)&)2-,)'*! ,%+,+! H?)A(-,)'*3! ,%61%(-,9(%! JJJI!@%(%!2-(()%7! '9,! -,! ,/%!5-<! \.-*G! V*+,),9,%! &'(! O<,(-,%((%+,()-.! \/=+)2+! )*!T%(6-*=! -*7! -,! ,/%! F/9*8#0/-*!V*+,),9,%!'&!02)%*2%!-*7!;%2/*'.'8=!HF0V0;I!)*!;-)@-*>!,/%!.-,,%(!'&!@/)2/!-.+'!6-*9&-2,9(%7!6'+,!'&!,/%!%.%2,('*)2!9*),+J!!!

!

$%-6! O*%(8=!H5%_I!

N%! P[E!

49! DBE!

i(! DKE!

Table 1.1: Beam characteristics used for AMS-01 electronic component tests at Dubna.

Page 26: 2004 Ams Nim Paper Draft

AMS-01/Electronics

!"#"E!

!

DAQ Switch

S2

Tracker

S4

CoincLevel-1

ORPlane Discr

PMT+HV

Trigger

ComputerLevel-3

Earth

Level-1

Level-2

ADC

DAQTrack

PMT+HV TDC,ADC

Readout

S1

S3

LatchHitEncode

Level-2Deflection

(1100/plane)

(3) (6) (8)

(3) (3) (3)

(3)

(3)

(4) (3) (4-8)

(3)

(3)

(3)

(3) (3)

(3)

(5)

Processor

!

Figure 1.14: AMS-01 electronics. The numbers of redundant elements are given parenthetically. !

Page 27: 2004 Ams Nim Paper Draft

AMS-01/Operations

! "#""

1.5 AMS-01 Operations 450#E"!@-+!.-9*2/%7!'*!,/%!0/9,,.%!Y)+2'?%(=!H0;0#e"!&.)8/,I!'*!P!j9*%!"eebJ!!Y9()*8!,/%!,%*#

7-=!6)++)'*!'&!Y)+2'?%(=3!450!@-+!-..'2-,%7!"EE!/'9(+!'&!1()6-(=!,)6%!,'!1%(&'(6!+=+,%6!,%+,+J! !;/%!(%+,! '&! ,/%! ,)6%3!Y)+2'?%(=!@-+! 9+%7! &'(! 7'2G)*8! -*7! ,(-*+&%(()*8! .'8)+,)2! +911'(,!@),/! ,/%!5Vh! +1-2%!+,-,)'*J!!M)89(%!"J"C!+/'@+!,/%!.)&,#'&&!'&!0/9,,.%!Y)+2'?%(=!@),/!450#E"!'*!A'-(7J!!;/%!1/','8(-1/!)*!M)89(%!"J"B3!,-G%*!&('6!5Vh!+/'(,.=!A%&'(%!7'2G)*83!+/'@+!450#E"!-,!,/%!(%-(!'&!,/%!0/9,,.%!2-(8'!A-=J!!!

!

!!

Figure 1.15: The launch of the Space Shuttle Discovery with AMS-01 on board.

Page 28: 2004 Ams Nim Paper Draft

AMS-01/Operations

!"#"P!

!

!Figure 1.16: Discovery with AMS-01 seen from MIR.

Page 29: 2004 Ams Nim Paper Draft

AMS-01/Physics

! "#"K

1.6 Physics results of AMS-01!M('6!,/%!0;0#e"!&.)8/,!'&!450#E"3!@%!8-)*%7!%<1%()%*2%!-*7!G*'@.%78%!'*!/'@!,'!%<%29,%!-!

1-(,)2.%!1/=+)2+!%<1%()6%*,!)*!+1-2%J!!;/%!2'*+,(92,)'*!'&!,/%!2'61.%,%!7%,%2,'(!@/)2/!@)..!A%!7%1.'=%7!'*! ,/%! 01-2%! 0,-,)'*! A%*%&),+! &('6! ,/)+! 1(-2,)2-.! 9*7%(+,-*7)*8! '&! ,/%! ,%2/*)2-.! 2-1-A).),)%+! -*7!1%(&'(6-*2%!'&!%-2/!2'61'*%*,!9*7%(!-2,9-.!&.)8/,!2'*7),)'*+J!

;@'! /'9(+! -&,%(! ,/%! +/9,,.%! .)&,#'&&! '*! P! j9*%! "eeb3! @%! A%8-*! 1%(&'(6)*8! ,%+,+! '*! 450J!!M)89(%!"J"[-! +/'@+! ,/%! '*#'(A),! 0).)2'*! ;(-2G%(! 7)+1.-2%6%*,! &('6! ,/%! 6%-+9(%6%*,! '&! ,/%! .-+%(!-.)8*6%*,! +=+,%6J! ! M)89(%!"J"[A! +/'@+! ,/%! +-6%! 6%-+9(%6%*,! @/%*! 450! @-+! '*! ,/%! .-9*2/! 1-7J!F'61-()*8! ,/%+%! ,@'! 6%-+9(%6%*,+! )*7)2-,%+! ,/-,! ,/%! (%.-,)?%! -.)8*6%*,! '&! ,/%! ,(-2G%(! .-=%(+! @-+!

6'*),'(%7!@),/!-*!-229(-2=!'&!K!-6J!!;/%!450!Y)8),-.!Y-,-!h%2'(7%(!@-+!-2,)?-,%7!)*!,/%!0/9,,.%!2(%@!2'61-(,6%*,!%*+9()*8!,/-,!-..!7-,-!@%(%!A%)*8!(%2'(7%7J!!!

!

98-06-0501:21:05centroid

at20 391.8 µm

on orbit

measureddisplacement:

1.1 µm ± 3 µm

160

165

170

175

180

185

190

195

200

205

210

215

3000

2500

2000

1500

1000

500

0

on pad

16

0

16

5

17

0

17

5

18

0

18

5

Si strip no. (110 µm per strip)

(a) (b)

Ave

rag

e p

uls

eh

eig

ht

(ad

c c

han

nels

, m

ip~

40

)

19

0

19

5

20

0

20

5

21

0

21

5

0

500

98-05-1412:05:05centroid

at 20 390.7 µm

1000

1500

2000

2500

3000

!

Figure 1.17: Laser displacement measured in orbit (a) and on launch pad (b).

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

4&,%(! ,/%! &.)8/,3!450#E"!@-+!2/%2G%7!-8-)*J! !;/%!7%,%2,'(!@-+!1.-2%7! )*! -!/%-?=! )'*! HR%3!FI!A%-6!&('6!"JE!,'!CJB!T_!-,!BEE!7)&&%(%*,!)*2)7%*,!-*8.%+J!!;/)+!,%+,!@-+!7'*%!@),/!-!,',-.!'&!DC!6)..)'*!%?%*,+! -*7!@-+! 2-(()%7! '9,! -,!T0V#Y-(6+,-7,J! ! M)89(%!"J"b! +/'@+! ,/%! .'2-,)'*! '&!450!-,! ,/%!T0V! )'*!-22%.%(-,'(!-*7!M)89(%!"J"e!+/'@+!'*%!'&!,/%!2-(A'*#A%-6!,%+,!(%+9.,+J!!!

4&,%(!T0V3!,/%!7%,%2,'(!@-+!1.-2%7!)*!-!1(','*!-*7!1)'*!A%-6!-,!FOhN3!@),/!6'6%*,96!&('6!P!,'!"D!T%_!-,!"PEE!7)&&%(%*,!)*2)7%*,!-*8.%+J!!;/)+!,%+,!@-+!7'*%!@),/!-!,',-.!'&!"EE!6)..)'*!%?%*,+J!

;/%!2'*,)*9%7!6'*),'()*8!'&!450#E"!2'*&)(6%7!,/-,!,/%!7%,%2,'(!1%(&'(6-*2%!A%&'(%3!79()*8!-*7!-&,%(!,/%!&.)8/,!(%6-)*%7!,/%!+-6%J!!V*!1-(,)29.-(3!,/%!-.)8*6%*,!%(('(!'&!,/%!+).)2'*!,(-2G%(!@-+!2'*,('..%7!

,'!A%!.%++!C!-6!,/('98/!'9,J!

Page 30: 2004 Ams Nim Paper Draft

AMS-01/Physics

!"#"D!

AMS

October 1998

!!

Figure 1.18: Location of AMS at the GSI Ion Accelerator.

GSI Carbon-beam

( peaks at Z=1 and 2 are

proton and helium

background )

Z

Eve

nts

0

100

200

300

400

500

600

0 1 2 3 4 5 6 7 8 9 10

p He

C

!

Figure 1.19: Results of tests of AMS-01with the GSI carbon beam.

Page 31: 2004 Ams Nim Paper Draft

AMS-01/Physics

! "#"C

;/'98/! ,/%! &)(+,! &.)8/,! @-+! -*! %*8)*%%()*8! &.)8/,3! '?%(! "EE!6)..)'*! %?%*,+! @%(%! 2'..%2,%7J! ! V*!-77),)'*!,'!?-.)7-,)*8!,/%!450!2'*2%1,3!-*-.=+)+!'&!,/%+%!%?%*,+!.%7!,'!,/%!&'..'@)*8!+)8*)&)2-*,!(%+9.,+:!

+ Search for antihelium in cosmic rays 4!,',-.!'&!PJbB!<!"EB!/%.)96!*92.%)!@),/!()8)7),)%+!91!,'!"DE!T_!@%(%!'A+%(?%7J!!N'!-*,)/%.)96!

*92.%)!@%(%!7%,%2,%7!-,!-*=!()8)7),=J!!;/%!6'+,!1(%2)+%!911%(!.)6),!'*!,/%!(-,)'!'&!,/%!&.9<!'&!-*,)/%.)96!,'!,/%!&.9<!'&!/%.)96!'&!.%++!,/-*!"J"!<!"E!B!)+!'A,-)*%7J!

+ Protons in near earth orbit ;/%! 1(','*! +1%2,(96! )*! ,/%! G)*%,)2! %*%(8=! (-*8%! EJ"! ,'! PEE! T%_! @-+! 6%-+9(%7J! ! 4A'?%! ,/%!

8%'6-8*%,)2! 29,'&&3! ,/%! 'A+%(?%7! +1%2,(96! )+! 1-(-6%,%()`%7! A=! -! 1'@%(! .-@J! !$%.'@! ,/%! 8%'6-8*%,)2!29,'&&3! -! +9A+,-*,)-.! +%2'*7! +1%2,(96!@-+! 'A+%(?%7J! !5'+,! '&! ,/%+%! +%2'*7! +1%2,(96! 1(','*+! &'..'@! -!2'61.)2-,%7!,(-W%2,'(=!-*7!'()8)*-,%!&('6!-!(%+,()2,%7!8%'8(-1/)2!(%8)'*J!!

+ Leptons in near earth orbit!;/%!.%1,'*!+1%2,(-!)*!,/%!G)*%,)2!%*%(8=!(-*8%+!EJP!,'!DE!T%_!&'(!%!!-*7!EJP!,'!K!T%_!&'(!%k!@%(%!

6%-+9(%7J! !M('6!,/%!'()8)*!'&!,/%!.%1,'*+!,@'!7)+,)*2,!+1%2,(-!@%(%!'A+%(?%7:!-!/)8/%(!%*%(8=!+1%2,(96!-*7!-! +9A+,-*,)-.! +%2'*7!+1%2,(96!@),/!1'+),('*+!692/!6'(%!-A9*7-*,! ,/-*!%.%2,('*+J! !;(-2)*8! .%1,'*+!&('6! ,/%! +%2'*7! +1%2,(-! +/'@+! ,/-,!6'+,! '&! ,/%+%! .%1,'*+! ,(-?%.! &'(! -*! %<,%*7%7! 1%()'7! '&! ,)6%! )*! ,/%!8%'6-8*%,)2!&)%.7!-*7!,/-,!,/%!%k!-*7!%!!'()8)*-,%!&('6!,@'!2'61.%6%*,-(=!8%'8(-1/)2!(%8)'*+J!!

+ Cosmic protons:!;/%!1(%2)+%!1()6-(=!1(','*!+1%2,(96!)*!,/%!G)*%,)2!%*%(8=!(-*8%!EJP!,'!PEE!T%_!@-+!-229(-,%.=!

6%-+9(%7J!!V,!)+!-*!)61'(,-*,!)*19,!,'!-,6'+1/%()2!*%9,()*'!%+,)6-,)'*+J!

+ Helium in near earth orbit:!;/%! /%.)96! +1%2,(96! &('6! EJ"! ,'! "EE! T%_]*92.%'*! @-+! 6%-+9(%7J! ! 4A'?%! ,/%! 8%'6-8*%,)2!

29,'&&3! ,/%!+1%2,(96!)+!1-(-6%,%()`%7!A=!-!1'@%(! .-@J! !$%.'@!,/%!8%'6-8*%,)2!29,'&&3!-!+%2'*7!/%.)96!+1%2,(96!@-+!'A+%(?%7J!!V*!,/%!+%2'*7!/%.)96!+1%2,(-!'?%(!,/%!%*%(8=!(-*8%!EJ"!,'!"JP!T%_]*92.%'*3!)*!,/%!8%'6-8*%,)2!.-,),97%!&('6!lEJD!,'!kEJD!(-73!,/%!&.9<!@-+!6%-+9(%7!,'!A%!HBJK!mEJeI!<!"E!K!]H6P+%2!+(I!-*73!2'*,(-(=! ,'!%<1%2,-,)'*+3!6'(%! ,/-*!*)*%,=!1%(2%*,!'&! ,/%!/%.)96!@-+!7%,%(6)*%7! ,'!A%!KR%!H-,! ,/%!eE^!FJZJIJ!

+ Deuterons in near earth orbit:!4! ,',-.!'&!"!<!"ED!7%9,%()96!*92.%)! )*! ,/%!%*%(8=! (-*8%!EJ"! ,'!"JE!T%_]*92.%'*!@%(%!'A+%(?%7!

-..'@)*8!,/%!&)(+,!-229(-,%!!,%+,!'&!8-.-2,)2!2'*&)*%6%*,!6'7%.+J!!

+ Search for antideuterium in cosmic rays: !V*! -! ,',-.! '&! "! <! "ED! 7%9,%()96!*92.%)! )*! ,/%!6'6%*,96! (-*8%! "! ,'! K!T%_]2! *'! -*,)7%9,%()96!

*92.%)!@%(%!7%,%2,%7!-,!-*=!6'6%*,96J!!;/%!6'+,!1(%2)+%!.)6),!'*!,/%!&.9<!'&!-*,)7%9,%()96!'&!.%++!,/-*!

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Page 32: 2004 Ams Nim Paper Draft

!

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2-1

Chapter Two: AMS-02, particle physics

on the International Space Station

AMS is scheduled to be installed on the Space Station in April 2007 for a period of three to five

years. This configuration of AMS, AMS-02, is shown in Figure 2.1. As will be described in the

following sections, the construction of the detector is progressing well. Because this is the major

scientific experiment on the Space Station, NASA is following the progress of AMS with detailed reviews

concerning the design and construction, safety and ground operations to ensure the detector can be

launched in April 2007.

Figure 2.1: The Alpha Magnetic Spectrometer (AMS) as it will appear on the ISS (AMS-02).

In addition to the detector elements of Figure 2, this figure shows the structural interface

(USS) which connects the detector to the shuttle and to the ISS, the thermal radiators, debris

shields, the electronics crate racks and the location of the Cryomagnet Avionics Box (CAB).

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2.1 Cryomagnet

The purpose of the superconducting magnet is to extend the energy range of our measurements of

particles and nuclei to the multi-TeV region [1,2]. The AMS-02 magnet design is under the overall

responsibility of ETH-Zürich and MIT. The magnet design was based on the following technical

considerations:

(i) Experience in designing and manufacturing the AMS-01 magnet which was 10 times safer than

stress limits allowed.

(ii) The result of many years of intensive R&D collaboration between ETH and the R&D group of

Oxford Instruments Ltd. to design a magnet with the following properties :

+ Identical field configuration to the AMS-01 magnet to maintain mechanical stability and

follow NASA safety standards, as shown in Figure 2.2.

+ Minimized heat loss (~100 mW) and minimized quench probability.

-100.0

-50.0

X

X

Y-100.0

Y-50.0

Y50.0

Y100.0

BL2=0.86 Tm2

1 2

3

4

5

6

7

8

9 10 1

1 12 13 14 15

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!!

!!!!

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!!

!!!!!!!!

BL2=0.14 Tm2

Both haveAMS-01 AMS-021- Same inner radius

2- Dipole moment = 03- B at 2.0 m ! 300 G

Figure 2.2: Identical magnetic field configuration between AMS-01 and AMS-02 magnets.

(iii) We have chosen to have the magnet built by experts from the Oxford Instruments R&D group,

who have an excellent record to produce highly reliable magnets running in persistent mode

without quench. This group has produced the 8 OSCAR magnets (2.36 Tesla) used in cyclotrons

in Japan and England and which have operated for close to 30 years without any quench. This

group also built the CLEO magnet at CORNELL and the CLAS torus at Jefferson Laboratory and

the KLOE magnet in Frascati. All are large, high-field, special-purpose magnets which have

operated for years without quench.

To ensure that these experts are able to devote all their efforts to the construction of the AMS-02

magnet, we have supported a new company: Space Cryomagnetics Ltd., entirely staffed by the

experts of the Oxford Instruments R&D group and entirely dedicated to the AMS-02 magnet.

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2-3

(iv) Most importantly, we are using a new, small cross-section, aluminium stabilized conductor

developed and mass-produced by the ETH-Zurich magnet group [1,2]. Based on test results, this

conductor reduces the quench probability by a factor of 2000. ETH has pioneered many of the

key technologies for producing Al stabilized conductors [1,2,3]. Aluminium stabilized conductor

is now widely used in high energy physics (HEP) detectors [4]. Figure 2.3 shows the non-

destructive quality control apparatus developed at ETH. It consists of an ultrasonic phased array

which ensures the continuous bonding between the superconductor and the high purity Al (see

Figure 2.7). It also includes a laser dimension measuring system and an eddy current check for

quality control. The system shown in Figure 2.3 ensures that Al stabilized superconducting cable

can be produced uniformly and reliably with lengths up to 2.5 km.

Figure 2.3:Technology developed at ETH for producing

high quality Al stabilized superconducting cable.

Two identical magnets are being built. One is the flight magnet and the other is used for space

qualification tests. The magnet has no magnetic field during the shuttle launch and landing and so there is

no force among the coils, hence for the test magnet the coils are replaced by mass equivalents.

The magnet system [1], as shown in Figures 2.4 and 2.5, consists of superconducting coils, a

superfluid helium vessel and a cryogenic system, all enclosed in a vacuum tank. Outside of the vacuum

tank are supporting electronics, located in the Cryomagnet Avionics Box (CAB), valves and cabling. The

vacuum tank is toroidal with inner diameter of 1.1 m, outer diameter of 2.7 m and a length of the central

cylinder surrounding the tracker of 0.9 m.

The magnet operates at a temperature of 1.8 K, cooled by superfluid helium stored in the vessel.

It is launched at the operating temperature, with the vessel full of 2500 litres of superfluid helium. The

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2-4

magnet will be launched with no field, it will be charged only after installation on the ISS. Because of

parasitic heat loads, the helium will gradually boil away throughout the lifetime of the experiment. After

the project time of 3 to 5 years, the helium will be used up and the magnet will warm up and no longer be

operable.

Figure 2.4: AMS-02 superconducting magnet layout.

VCS3

VCS2

VCS1

VCS4(68K)

BB

COLD HEATEXCHANGER

NON-LINEARSTRAPS

CRYOCOOLERS (4)

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ø2.5m

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+Y

+X +Z

LC

He2 TANK (1.6K)

3.0 mmMIN THICK He2

He2

CoilCoil

8600 G

Figure 2.5: Sectional view of the AMS-02 superconducting magnet (VCS – Vapor Cooled Shield).

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2-5

2.1.1 Magnet Coil System

The coil system consists of a set of 14 superconducting coils arranged, as shown in Figure 2.4,

around the inner cylinder of the vacuum tank. The coil set has been designed to give the maximum field

in the appropriate direction inside the bore tube, while minimising the stray field outside the magnet.

As seen from Figure 2.6, the single large pair of coils generates the magnetic dipole field

perpendicular to the experiment axis. The twelve smaller flux return coils control the stray field and, with

this geometry, they also contribute to the useful dipole field. Figure 2.6 also shows the strength and

direction of the magnetic field within the set of coils. The magnetic flux density at the geometric centre

of the system is 0.86 T. Table 2.1 summarizes some of the magnet parameters.

Figure 2.6: Coil arrangement of the AMS-02 superconducting magnet, showing the two large dipole

coils and the 12 smaller flux return coils and the field map inside the magnet bore.

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Central Magnetic Field Bx (0,0) [T] 0.860

Dipole Bending Power [Tm2] 0.862

Maximum Stray Magnetic Field at R=2.3 m [mT] 15.2

Maximum Stray Magnetic Field at Y=2.3 m [mT] 7.6

Maximum Stray Magnetic Field at R=3.0 m [mT] 3.9

Peak Magnetic Field on the Dipole Coils [T] 6.59

Peak Magnetic Field on the Racetrack Coils [T] 5.91

Maximum Torque in geomagnetic field [Nm] 0.272

Nominal Operating Magnet Current [A] 459.5

Stored Energy [MJ] 5.15

Nominal Magnet Inductance [H] 48

Table 2.1: AMS-02 Cryomagnet parameters.

The superconducting wire for the AMS magnet was developed specifically to meet the

requirements of the AMS cryomagnet by ETH-Zürich [2]. The current is carried by tiny (22.4 -m

diameter) filaments of niobium titanium (NbTi) which - given the magnetic flux and current densities

within the coils – carries the current without resistance provided the temperature is kept below 4.0 K.

Because pure NbTi has rather low thermal conductivity, it is prone to instability. This can be overcome if

it is in intimate contact with a material which has a high thermal conductivity at the cryogenic operating

temperature, such as a pure metal. For this reason, the NbTi filaments are embedded in a copper matrix,

which is encased in high-purity aluminium. The copper is required for manufacturing reasons, but the

aluminium is extremely conductive and much less dense, thus providing maximum thermal stability for

minimum weight.

Figure 2.7 shows a cross section of the aluminium-stabilized conductors developed by the ETH

group and a magnified section through the wire. The diameter of the round copper strand at the centre is

0.76 mm, and the aluminium dimensions are 2.0 mm x 1.5 mm. The current density in the

superconductor is 2300 A/mm2 or 157 A/mm2 including the aluminium.

To manufacture the coils, the superconducting wire was first cleaned then insulated using 85 -m

thick polyester tape. Each coil was wound separately onto an aluminium former from a single length of

conductor before being impregnated under vacuum with epoxy resin. The impregnation process gives the

coils mechanical integrity, and also provides electrical insulation between turns and layers. After

completion, each coil is tested individually under conditions as representative as possible of flight, to test

the integrity of the design and the quality of the build, as shown in Figure 2.8.

Each of the two larger (dipole) coils, which generate most of the useful field, has 3360 turns, and

the 12 smaller (flux return) coils each have 1457 turns. The 14 coils are connected in series, with a single

conductor joint between each pair of adjacent coils. The current when the magnet is operating is 459.5 A.

All of the coils have been manufactured and tested (see Figure 2.9).

If magnet coils are not well designed, heating in a quench can be so rapid that the conductor may

actually melt in the region where the quench began. Another problem can occur in systems consisting of

a number of coils, where quenching of one coil - and the collapse of its associated magnetic field – can

lead to increased current flow and field in other coils coupled by mutual inductance. In some cases this

can lead to excessive stresses within the windings and between the coils.

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2-7

Figure 2.7: Cross sections of the Aluminum stabilized NbTi/copper composite conductor.

Dimensions in mm.

Figure 2.8: Testing the coils to flight loads.

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2-8

Figure 2.9: Arrangement of the completed 2 dipole coils, 12 flux return coils and structural

members in roughly the positions they will have in the flight magnet.

The AMS magnet has been specifically designed to avoid these hazards. The aluminium-

stabilised conductor is sufficiently conductive that the coils are very stable. If a quench does occur, the

heat generated is conducted throughout the coil so quickly that the peak temperatures reached are not

hazardous. Because all 14 coils are connected in series they have to carry the same current at all times, so

there is no danger of magnetically induced stresses causing damage. However, the coils are not very

closely coupled thermally. This means that a quench in one coil, leading to a rise in temperature, will not

necessarily propagate to any of the others. If this were allowed to happen, the entire stored energy of the

magnet (5 MJ) could be dissipated as heat in the coil which quenched. While the temperatures reached in

that coil would not be dangerous, sufficient thermal stresses could be induced (by differential thermal

contraction between parts of the coil) that the performance of the coil might be permanently reduced. For

this reason, all the coils are constantly monitored by an electronic protection system. If the onset of a

quench is detected in any coil, heaters are powered in the other coils to quench all 14 simultaneously.

This distributes the stored energy between the coils, preventing any single coil from taking a

disproportionate amount of energy which could otherwise result in degradation. The operation of these

quench heaters is an important part of the testing and qualification procedure for the magnet coils.

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2-9

2.1.2 Mechanical System

The mechanical loads on the system are either magnetic or inertial. Magnetic loads apply

whenever the magnet is charged, and can be between or within coils. Significant inertial loads are applied

during launch, re-entry and landing of the Space Shuttle. But, because the magnet will not be charged

during launch or landing, magnetic and inertial loads are never superimposed.

In general, the magnetic loads are much greater than the inertial loads. All magnetic loads are

reacted within the structure of the coil set, and none are transmitted to the vacuum tank or other parts of

the AMS system. These loads are resisted by components made from high strength aerospace grade

aluminium alloy, chiefly 6061-T6.

Each coil is subject to internal forces as a result of its own magnetic field. In general, these are

burst forces, trying to expand the racetrack-shaped coil into a ring. These loads are in the plane of the

coil, and are resisted by the former on which the coil was wound. In addition, each coil is attracted or

repelled by all the other coils in the magnet. This leads to a relatively complicated load system on some

of the coils, with forces perpendicular to the plane of the coil.

The magnetic loads are quite large: the two dipole coils feel a net attraction to each other of

around 250 tonnes. During individual coil testing, each coil is charged until some part of the winding is

subject to the same force it will experience in flight.

The cold mass of the magnet is more than 2000 kg. This has to be supported from the experiment

structure (in particular the vacuum tank), which is at ambient temperature (~270/40 K). The design of

the support straps is therefore crucial, as they have to be able to carry the load without conducting

significant heat across the large temperature gradient.

During normal operation on the ground, inertial loads are relatively small: once on orbit they

disappear altogether. At these times, the function of the straps is only to position the magnet correctly

within the vacuum tank. During launch and landing, however, inertial loads and vibration become very

significant. Now the straps have to resist large forces, and also require high stiffness to prevent low

frequency resonance which could lead to mechanical damage.

For high strength and stiffness, the straps need large cross-sections. However, this inevitably

leads to high levels of heat conduction, which would reduce the endurance of the superfluid helium

system and thus shorten the life of the experiment. For minimum heat conduction, the straps need to be

very thin, but this gives poor strength, low stiffness and a low resonant frequency.

The straps have been designed to satisfy all of these requirements. Each consists of a pair of

composite bands connected in parallel. One band is thin, with low stiffness and strength, and is

permanently connected between the cold mass and the vacuum tank. The other band is much thicker and

stronger, but possesses a passive disconnect feature. This means that it only forms a thermal path

between the vacuum tank and the magnet during launch and landing. At other times (when it is not

needed), differential thermal contraction between the bands and the removal of the high inertial load

cause the disconnect to open, dramatically reducing the thermal conduction of the support.

A total of 16 straps support the magnet from the vacuum tank (see Figure 2.10). During normal

operations on the ground or in space, only the low-stiffness band is engaged, and the heat conduction is

very low (less than 3 mW per support). During launch, the high-stiffness band engages as well. The

conducted heat load is much higher but because the launch takes only a few minutes the effect on the

overall endurance of the system is not significant.

The dual stiffness characteristic of the straps makes their behaviour non-linear and, as major

structural components of the magnet system, they have been subject to special scrutiny and testing,

particularly testing to failure to understand the safety margins (see Figure 2.11).

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Figure 2.10: The Magnet support straps. The cold mass at 1.8 K has to be supported to the vacuum

case which is at approximately 270 K. This is achieved by 16 straps, which hold the 2 ton

cold mass in position during launch (acceleration 3g) and landing (deceleration 10g). In

space, the straps are designed to be nearly disconnected so as to not transfer heat from the

vacuum case to the cold mass.

Figure 2.11: .Testing of strap to failure to understand the critical failure mode.

Assembly failure caused by failure of the glass fiber “bod”, other damage

observed caused by impact loading as strap failed, not by static loading.

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2.1.3 Cryogenic System

The cooling of terrestrial superconducting magnets using liquid helium is a well-established

technology, but there is little experience of helium cryogenics in space. Apart from a few very small-

scale experiments, the only major missions involving liquid helium have been the Infrared Astronomical

Satellite (IRAS) [5], the Cosmic Background Explorer (COBE) [6], the Infrared Space Observatory

(ISO) [7] and the Superfluid Helium On-Orbit Transfer demonstration (SHOOT) [8].

The cryogenic system for the AMS magnet combines technologies from terrestrial magnet

cryogenics and space cryogenics to meet the particular challenges of the Space Shuttle launch and the

environment of the ISS [9]. It maintains the magnet at a temperature of 1.8 K, under all operating

conditions, for the duration of the experiment. It therefore has to be able to store enough helium to last

the entire mission, to transfer any heat from the cold components to the helium, to allow the magnet to be

charged and discharged safely from the external power supply, and to re-cool the magnet after a quench.

On the ground, it also has to control the cool down of the magnet from ambient temperature.

Figure 2.12 shows all the elements of the AMS-02 cryogenics system, including the passive

phase separator (PPS), which removes the gaseous He which is then used to cool the 4 vapour cooled

shields, the two thermo-mechanical pumps (TMP), one to cool down the magnet in the unlikely event of a

quench and the other to cool down the current leads during magnet charging and discharging, the helium

gas pressure activated cold valves which operate at 1.8 K, the warm valves outside the vacuum tank

which operate at ambient temperature but with cold He gas flowing through them and the burst disks (0.8,

3, 10 and 20 bar) for safety. The valves are implemented redundantly in parallel (for example DV06A,

B), or series (DV16A, B) or both (DV15A, B, C, D).

i) Helium Management and Endurance

Liquid helium (4He) can exist in two forms. Normal liquid helium behaves in a conventional

manner. But if it is cooled below 2.17 K, some of its properties change dramatically as it becomes a

superfluid. In particular, its viscosity falls almost to zero, and its apparent thermal conductivity increases

by many orders of magnitude.

The AMS magnet is cooled by superfluid helium. There are two main reasons for this. Firstly,

the specific latent heat and density of superfluid helium are both higher than in normal liquid helium.

Since the amount of cryogen that can be carried is limited by the size of the helium vessel, this gives a

useful endurance benefit (there is a greater mass of helium, and each kilogram has a higher cooling

capability). Secondly, in zero gravity there can be no convection currents. In normal liquid helium this

can result in thermal stratification, making it difficult to ensure that all parts of the system are fully cold.

In the superfluid state, however, the very high thermal conductivity makes it impossible for the helium to

support large temperature gradients, so the system remains isothermal.

Superfluid helium is obtained by reducing the pressure above a vessel of normal liquid helium.

The boiling point of helium at atmospheric pressure is 4.2 K, and this can be reduced to 1.8 K if the

absolute pressure is reduced to 16 mbar. On the ground, this pressure reduction is achieved using large

vacuum pumps to remove helium vapour. Once on orbit, the vacuum of space itself is used as a pump,

and the low temperature can be achieved simply by venting the helium vessel to space.

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2-12

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2-13

ii) Helium Vessel

The helium vessel is a toroidal tank, with inner and outer diameters of 1.92 m and 2.58 m, length

1.18 m and volume 2500 litres. It is a fully welded construction of aluminium alloy 5083-H321. For

maximum strength and minimum weight, both cylinders are ribbed and they are joined together by cross-

bracing at the mid-plane.

The sixteen support straps have to pass through the volume occupied by the helium vessel as they

support the coils from the outer cylinder of the enclosing vacuum tank. Because a high heat load would

result if the straps came into contact with the helium itself, the vessel is equipped with 16 tubes which

pass completely through it. These allow the straps to pass through the vessel while remaining in vacuum.

Figure 2.13 shows the construction of the vacuum tank and Figure 2.14 shows the welding of the

He tank.

Figure 2.13: Construction of the vacuum tank, also showing the location of the support straps.

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2-14

Figure 2.14: Welding of the He tank.

iii) Phase Separation

The heat which leaks into the system is transferred to the helium in the 2500 litre vessel, which is

the ultimate low temperature heat sink for the system where the heat is dissipated by boiling the

superfluid helium. For efficient use of the helium, the gas which is generated has to be separated from the

liquid and used to remove heat from other parts of the system. On the ground, phase separation can be

achieved simply by placing the vapour vent at the highest point in the vessel: gravity will then ensure that

the liquid remains at the bottom and the vapour is released from the top. In space this approach clearly

will not work, so the system uses a special zero-gravity passive phase separator (PPS) [10] developed by

Linde in Germany. The phase separator is similar in construction to that used on ISO, consisting of a

porous plug of sintered stainless steel in a steel housing. In flight, a slight (~30 mK) temperature

difference is maintained between the two faces of the plug. The separator takes advantage of the thermo-

mechanical effect [11] that superfluid He liquid moves from cold regions to hot regions, thus the He gas

can be removed and the superfluid He liquid retained, see Figure 2.15. The phase separator for AMS has

been tested (see Figure 2.16) and is ready for welding into the helium vessel.

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2-15

GasColder

Warmer

Coils

Coils

Cold Heat ExchangerCold Heat Exchanger

Passive Phase Separator (PPS)

"T = 0.030KHe cannot escape.

SuperfluidSuperfluidHeHe

Figure 2.15: Schematic of the principal of phase separation as used in AMS-02.

Figure 2.16: Passive phase separator under test at Linde, Germany.

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2-16

iv) Vapour Cooled Shields (VCS)

A series of four concentric shields completely encloses the magnet and helium vessel (see

Figure 2.5). By cooling these shields with the vapour from the helium vessel (separated by the phase

separator, PP), the heat leak into the coldest parts of the system is dramatically reduced, and thus the

lifetime of the experiment increased. The vapour flows through pipes connected to the shields, removing

radiated heat as well as intercepting conducted heat from the support straps and other components.

The design of the shields is particularly challenging, as there is very little space available for

them. To maximise the useful field in the bore of the magnet system, the coils have to be large, and also

as close as possible to the inner surface of the vacuum tank. Likewise, the helium vessel has to be large

to be able to carry the maximum volume of superfluid helium.

Two of the shields are rigid, consisting of variable-thickness aluminium honeycomb with

fibreglass skins. These are designed for minimum thickness while retaining sufficient strength to

withstand launch and landing loads. The other two shields are flexible, made from thin sheets of soft

aluminium. Figure 2.17 shows one of the completed (honeycomb) shields.

Figure 2.17: One of the four vapour cooled shields ready for installation.

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v) Cryocoolers

Cryocooler technology has made great progress in recent years but, for fundamental

thermodynamic reasons, coolers capable of reaching temperatures approaching 1.8 K require extremely

large amounts of power at ambient temperature to be able to provide significant cooling. This power is

not available on the ISS, so it is not feasible to provide mechanical cooling to the magnet itself.

However, the heat load to the 1.8 K parts of the system can be reduced significantly if heat is removed at

a higher temperature.

For this reason, four Stirling cycle coolers are connected to the outer vapour cooled shield. The

coolers are qualified and tested (see Figure 2.18) by a team at NASA Goddard Space Flight Center, and

are expected to remove a total of about 12 W at 68 K. This should be sufficient to reduce the rate of

consumption of superfluid helium by a factor of four. A high (~92%) efficiency power supply to drive,

control and monitor the coolers has been developed by ETH-Zürich, MIT and RWTH-Aachen. One of

the initial concerns over the cryocoolers was whether their performance might be compromised by the

presence of the magnetic field. However, testing carried out by NASA at MIT [12] has demonstrated that

the cryocoolers can be operated without problems or degradation in the stray field generated by the

magnet in the locations where they are installed.

Each cooler consumes 100 W, which, along with the heat removed from the cryogenic system, is

conducted using a dual redundant capillary pumped loop to a quarter panel zenith facing radiator on the

top of the experiment (see § 2.9).

Figure 2.18: Vibration test of Cryocooler at NASA-GSFC.

vi) Mass Gauging

In zero gravity there is no clearly defined liquid level, so conventional helium level probes cannot

be used. Instead, a calorimetric method is used to determine the mass of helium in the tank. Detailed

analysis of this technique has been published [13] but the principle is simple. A small heat pulse is

applied to the helium while the temperature is monitored some distance away in the vessel by an accurate

thermometer. Because of the high thermal conductivity of the superfluid, the helium in the vessel is

isothermal. The heat pulse is therefore manifest not by local boiling of helium but by a small rise in the

temperature of the entire helium bath, measured by the thermometer. Knowing the energy dissipated by

the heater and the temperature rise in the bath, the mass of helium can be deduced.

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The mass gauging system for AMS is similar to the one used on ISO [7] and has been developed

by Linde, Germany. The performance depends critically on the accuracy of the temperature

measurement, and is therefore limited by the electronics. Two redundant mass gauges will be used on

AMS. Both have been tested and qualified.

vii) Coil Cooling System

The most obvious feature about the cooling system is that the coils are dry; they are not mounted

inside the helium vessel, see Figure 2.19. There are two reasons for this. Firstly, if the coils were inside

the helium space, the geometry of the vessel itself would become very complicated, and this would add

considerable mass. Secondly, and more importantly, it must be possible to recover from a magnet quench

in space (however unlikely this may be) by re-cooling the magnet using the onboard helium. If a magnet

immersed in helium quenches, the heat transfer is so rapid that the helium quickly pressurises and is lost

through the vessel pressure relief devices.

Figure 2.19: Arrangement of the coils surrounded by the He tank.

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If the coils cannot be physically inside the helium vessel, they must be cooled instead by

conduction to the superfluid helium. The ideal conductor would have very high thermal conductivity at

very low temperatures (to remove steady state and charging heat loads from the coils) but much lower

conductivity at higher temperatures (to avoid transferring heat too quickly to the superfluid following a

quench). Fortunately, helium itself fulfils both these requirements, having extremely high thermal

conductivity below 2.17 K but relatively low conductivity above this temperature.

The coil cooling scheme, based on this principle, is shown schematically in Figure 2.20. Each

coil is connected at two positions to a thermal bus bar which consists of a copper pipe filled with

superfluid helium. This helium is at a pressure of around 1 bar, so that it is supercooled and boiling is

suppressed. Part of the thermal bus bar is inside the main superfluid helium vessel and so acts as a heat

exchanger (see Figure 2.12). Heat radiated to (or generated in) the coils is transferred by Gorter-Mellink

conduction (the heat transfer mechanism in superfluid helium) through the superfluid helium in the

thermal bus bar and is dissipated by boiling the helium in the vessel.

The copper pipe forms a sealed circuit, filled with helium while the magnet is being cooled down,

but there is no net flow through it. Analysis of the flow of heat around the thermal bus bar requires the

solution of the non-linear differential equations describing Gorter-Mellink conduction. The methodology

used in this case was based on that developed by Mord and Snyder [14] and adapted for the AMS

geometry.

Figure 2.20: Principal of AMS-02 coil cooling system.

viii) Current Supply

The magnet can be operated at currents up to 459.5 A. It is equipped with persistent switches

which, when closed, form a superconducting link across the terminals of the magnet. This allows it to

continue to operate, once charged, in persistent mode without connection to the external power supply.

The leads, which supply current from the power supply to the magnet, are therefore only used for

charging or discharging: since the magnet will mostly be operated at a constant field, the leads will be

used only rarely.

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For this reason, the leads are designed for minimum heat leak when they are carrying no current.

This makes them less efficient during charging but, because their overall duty cycle is very small, results

in total in much reduced helium consumption. To achieve this, the cross section of the leads is relatively

small. When the magnet field is constant and the leads carry no current, the conducted heat load is

therefore minimised. During charging, the leads generate a substantial amount of Ohmic heating because

their resistance is rather high. This heat can only be removed by helium from the superfluid helium

vessel. However, the vessel itself operates at a pressure of just 16 mbar, which is not high enough to

ensure a sufficient flow of helium.

A thermo-mechanical pump (TMP) is therefore mounted in the superfluid helium vessel. The

TMP is used to pump helium from the vessel through the current leads to provide cooling when required

(see Figure 2.12). The TMP operates like the PPS in reverse. A small heater is used to induce a slight

temperature difference across the TMP, but with the warmer side towards the current leads and the cooler

side towards the He vessel, causing sufficient He to be pumped out to cool the leads. TMP technology in

space was first demonstrated by NASA in the SHOOT demonstration but the TMP for AMS differs in

details of its operation, and is developed by the Institut für Luft und Kältetechnik (ILK), Dresden,

Germany [15].

A further reduction in the heat conducted by the current leads when the magnetic field is constant

(no current through the leads) is given by a disconnect feature near the warm end of the leads. This

device provides a complete thermal and electrical break in the leads when the persistent switch is closed

(see Figure 2.21).

ix) Cryogenic Ground Support Equipment

To cool the magnet and fill the He tank a substantial amount of cryogenic ground support

equipment (CGSE) is being provided by Shanghai Jiao Tung University (SJTU), ETH, MIT and the

Kurchatov Institute. The 2 ton cold mass has to be cooled from 300 K to 1.8 K while maintaining a

temperature gradient of less than 50 K and the 2500 liter tank must be filled with superfluid He at a

pressure of 16 mbar. In addition, to support the installation and testing of AMS-02 in various locales (see

§ 2.10 and 2.11) the system must be portable. To maintain the reliability of the system, the system must

be very clean and the He filtered to 0.5 µm (nominal grade).

The CGSE scheme is depicted in Figure 2.21. Cooling proceeds in three phases: from 300 K to

90 K using liquid nitrogen externally to cool gaseous He which circulates through the internal system,

from 90 K to 4.2 K using gaseous and liquid He and from 4.2 K to the working point of 1.8 K by

pumping. From room temperature to the operational condition the three phases together are estimated to

take less than three weeks and require 2.4 tons of N2 and 1 ton of He. Subsequently the He tank can be

topped off, for example while AMS is installed in the space shuttle on the launch pad, using just the

equipment indicated. All equipment is manufactured under strict quality and cleanliness controls.

x) Cryogenic Safety

Any large cryogenic vessel has to be viewed as a potential safety hazard, particularly when it is in

an enclosed space such as the payload bay of the Space Shuttle. Safety of the AMS magnet has to be

assured in ground handling operations, during launch, on orbit and during landing. All cryogenic

volumes, as well as the vacuum tank, are protected by burst discs to prevent excessive pressures building

up in any fault conditions. Some of the burst discs have to operate at temperatures below 2 K, and these

have been the subject of a special development and testing programme.

In addition, extra protection is provided to mitigate the effect of a catastrophic loss of vacuum.

This could be caused, during ground handling operations, by a serious rupture of the vacuum case. If the

vacuum case had a large puncture, air could rush through the gap and condense on the surface of the

helium vessel. This would result in rapid pressurisation and venting of the helium in the vessel. To slow

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down the rates of pressurisation and venting (making the pressure relief path smaller and more

manageable) a 3 mm layer of lightweight cryogenic insulation will be applied to the outside surface of the

helium vessel. Carefully constructed experiments have shown that this insulation reduces the heat flux to

the superfluid helium by a factor of 8 following a sudden, total loss of vacuum.

Figure 2.21: Cryogenic Ground Support Equipment schematic. The equipment in

the upper right is also used to top off the He tank and is designed to be

compact and portable.

2.1.4 Cryomagnet Avionics

The electronics to power, monitor and control the magnet is housed primarily inside the

Cryomagnet Avionics Box (CAB) under the responsibility of CIEMAT and MIT. As illustrated in

Figure 2.22, this avionics includes:

a) the Cryomagnet Current Source (CCS) and precision shunt, used to charge the magnet,

b) the dump diode arrays mounted on the port and starboard USS (CDDP and CDDS), which

dissipate the energy stored in the magnet when it is ramping down,

c) the Cryomagnet Self Protection (CSP), used to detect and protect the magnet in case of a quench

or the loss of power or communications,

d) the dual redundant uninterruptible power supplies (UPS), which power the self protection

functions,

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e) the Cryomagnet Controller and Signal Conditioner (CCSC), which gather the monitoring data

from the rest of the avionics data and forwards it to the JMDC (see § 2.8) and receives and

executes commands from the JMDC,

f) the Power Switches module, which activates valves and heaters as directed by the CCSC, and

g) the Cryocooler electronics box (CCEB), (see § 2.1.3.v).

Figure 2.22 also shows the major electrical features of the magnet which include the

superconducting coils with a load of zero ohms and an inductance of 48 henries (see § 2.1.1), the

persistent switch and mechanical disconnecting current leads (§ 2.1.3.viii), the quench heaters (§ 2.1.1),

warm and cryogenic valves and associated temperature, pressure and voltage sensors (§ 2.1.3).

Additional sensors are located within the CAB itself.

Operationally, the magnet will be launched cold but at zero field and charged only after

installation on the ISS. Charged or not, the CCSC will continuously monitor the magnet state and relay

these readings through the AMS CAN bus housekeeping network to the JMDC. Altogether about 150

values are monitored including 23 prime and 23 redundant cryogenic temperature measurements based on

CERNOX sensors, which cover ranges from 1.4 to 400 K with accuracies down to 1 mK. These exacting

measurements allow the proper functioning of the cryogenics and magnet to be accurately controlled.

The information will then flow to ACOP, the AMS computer inside the ISS, and through the NASA air to

ground links to the POCC, the AMS ground operations center. Commands follow the reverse path to

reach the CCSC, which then initiates the appropriate action within the CAB and the magnet.

The magnet is charged by the CCS. After various checks to ensure, for example, that the magnet

coils are superconducting, the complete charging operation consists of five phases: preparation, output

voltage limited charging, power limited charging, current limited charging and disconnection. To prepare

the magnet for charging, the current leads are cooled by He vapor generated by the differentially heating

the associated TMP, the superconducting persistent switch is "opened" by heating it into the normal state

and the current leads are mechanically connected. The CCS then draws power directly from the ISS

120 VDC “A” feed and it is converted to a maximum of 10 VDC using six DC-DC converters in parallel.

The resulting current flows through the precision shunt to the current leads and serially through all the

magnet coils and back. In the third phase the power drawn from the ISS is limited to 1875 W and the

current in the coils continues to increase while the output voltage drops. Then the target coil current of

459.5 A, as monitored by the precision shunt is smoothly approached. After the target current is reached

the persistent switch is allowed to cool and it again becomes superconducting and the current is trapped

within the closed circuit of the magnet coils plus switch. Then the current leads are disconnected and no

longer need to be cooled by the TMP and the CCS is shutdown. In total the charging process is estimated

to take less then 2 hours.

Ramping down the magnet current is less complicated. The CCS remains powered off and

disconnected, the current leads are cooled and connected and the persistent switch is again driven open.

The current in the magnet coils then flows through the dump diodes (CDD-P,-S) which are mounted

directly on the Unique Support Structure (USS) and the stored magnetic energy is converted into heat

dissipated by these diodes. To dissipate the 5 MJ stored in the magnet is estimated to take less than

1.5 hours.

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Fig

ure

2

.22

: A

MS

-02

Cry

om

ag

net

Av

ion

ics

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The CSP has two overlapping functions: to detect and protect the magnet should a quench occur

and to automatically ramp down the magnet after a fixed delay should either power or communication to

the experiment be interrupted. As noted in § 2.1.1, an uncontrolled quench, though unlikely, could

damage the magnet. If the onset of a quench is detected, as indicated by a voltage drop anywhere over

the coils or persistent switch, a fast pulse of energy is required to fire the quench heaters wound within

each coil and dissipate the stored magnetic energy evenly over the cold mass. As the power level

required is never available from the ISS, this energy is drained directly from the UPS to the quench

heaters. If, during a charge or discharge operation, the current leads start to overheat, they can also be

damaged quite rapidly, so current lead temperature sensors are also tied into the quench heater trigger.

It should be stressed that, owing to the advanced properties of the AMS superconductor and the

cryogenics design, none of these conditions, including a spontaneous magnet quench, is anticipated to

occur on orbit. However, should it ever happen, this design ensures that the magnet will not be damaged

and that, after re-cooling, it can be recharged and the mission can proceed successfully. In any case, no

hazard will be presented.

When charged, the magnet current would continue to circulate indefinitely, even if the experiment

was powered down or the command path to the experiment was broken. To obviate concerns arising from

this when attached to the ISS, the CSP also contains an auto ramp down timer. In the event that no

external communication is received for 8 hours the CSP initiates the ramp down sequence, while

continuing to monitor and protect against a quench. Consequently, even in the event that power or

communication to AMS is interrupted, after 8+1.5 hours the magnet is guaranteed to be at zero field.

A critical element of the magnet avionics is then the Uninterruptible Power Supply (UPS), which

provides the power to the CSP and through the CSP to the quench heaters, in the unlikely event of a

quench. After an extensive investigation of capacitors and battery technologies it was determined that

only the highest quality Lithium-Ion cells would fulfill the requirements of energy density, thermal

operating range and rate of discharge, as well as reliable and safe operation on orbit. These cells are

being produced by Yardney/Lithion. They are based on the mechanical design space proven in the Mars

Lander and Exploration Rover programs and the cell chemistry used in the B2 Bomber upgrade. In

addition they are supplied with a Battery Management Systems (BMS) adapted for the AMS-02

requirements from a space qualified system developed for JPL. The BMS ensures that the eight cell

battery is neither over charged nor over discharged, both of which could reduce the battery capabilities,

though with the implemented mechanics and chemistry neither condition would be a hazard. However, as

even the highest reliability batteries may not perform at full capacity at end of life, two UPS (cell pack

plus BMS) will be installed on AMS-02. Either is sufficient to meet the requirements.

Owing to the amount of stored power and because the CCS within the CAB is connected directly

to the ISS power bus, detailed analysis has been done to ensure proper grounding and isolation, both

against possible breakdowns and against electromagnetic interference within the CAB, between the CAB

and the rest of AMS, and between the CAB and the ISS.

The level of space qualification required for the CAB project is significantly more stringent then

for the bulk of the electronics in AMS-02. From design and procurement through production and testing

the CAB will use space quality techniques. The entire CAB has been designed to be single fault tolerant

and certain critical blocks have been replicated to allow successful operation after multiple faults. For

example, should one of the six primary DC-DC converters fail in the CCS, the remaining five are

sufficient to reach full field. Even if a second converter were to fail, the field value could reach over 80%

of nominal. As another example, the target current is obtained by using the median result between three

independent circuits which compare the voltage drop measured across the precision shunt to a reference

voltage, where each circuit is fed by an independently generated reference. Also, the control, signal

condition blocks of the CCSC and the power switching are redundantly duplicated and cross strapped,

with the primary and redundant sides being independently powered with dedicated converters and

28 VDC feeds.

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2.1.5 Test Results

All parts of the AMS magnet system are subject to a battery of tests to ensure their quality and

integrity, and their suitability for the mission.

i) Coil Tests

Every one of the 14 superconducting coils will have been tested before assembly into the final

magnet configuration. All twelve of the flux return coils have been tested successfully, and the first of

the two dipole coils is undergoing final preparations for testing. A special test facility has been

constructed (Figure 2.23) which allows the coil to be operated under cryogenic conditions as close as

possible to flight. In particular, the coil is mounted in a vacuum space, and is cooled by a thermal bus bar

of the same construction as the one in the flight system.

Figure 2.23: Coil test facility.

Although the maximum current in the fully-assembled magnet system is 459.5 A, individual coils

are tested to different currents. This is because the distribution of magnetic field is different when a coil

is tested in isolation. The coils have therefore been tested at currents high enough that some part of the

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coil is subject to the same stress that it will experience in the full configuration. If the test current was

higher, then this part of the coil would be over-stressed. In practice, this means that some of the flux

return coils are tested at 600 A, others at 562 A and the dipole coils at 335 A.

The procedure for testing the flux return coils was to charge to the maximum current (600 A or

562 A), then reduce to 459.5 A. With the coil held at this current, the quench heater was powered at

200 W for a controlled time period. Heater pulses were applied in increments of 10 ms until the coil

quenched. After the quench, the coil was re-cooled and charged again to 459.5 A, to check that there was

no damage. The two dipole coils will follow a similar testing procedure. Completion of all coil testing is

expected in the first half of 2004.

ii) Coil Cooling System Tests

A full-scale replica of the superfluid thermal bus bar system outlined above was designed and

assembled. The replica consisted of a thermal bus bar in the form of a 20 m long sealed copper pipe with

a 15 mm bore. Part of the pipe was inside a 200 litre helium vessel to provide a cold heat exchanger: the

rest was in the vacuum space.

The copper pipe was connected to an external, clean supply of helium. The vessel was cooled

down and filled with liquid helium which was then further cooled to 1.8 K by pumping. Helium was

drawn into the copper pipe due to the cooling, but the pressure was maintained at around 1 bar.

Eventually, the 200 litre vessel contained boiling superfluid helium at 1.8 K and 16 mbar, and the pipe

was filled with supercooled helium at 1.8 K and 1 bar.

Heaters on the part of the thermal bus bar outside the helium vessel were then used to simulate

the heat load due to the magnet coils being charged. Up to 6 W could be generated by the heaters and

transferred by Gorter-Mellink conduction through the thermal bus bar to be dissipated in the vessel of

boiling helium. If the heaters were used to generate more power, the Gorter-Mellink conduction broke

down: the thermal bus bar was unable to transfer the heat and the temperatures within it began to rise

rapidly. These results corresponded to the calculations carried out before the tests.

iii) Cryogenic Safety Tests

A series of experiments has been carried out to determine what happens in the event either of a

catastrophic loss of vacuum or of a much smaller vacuum leak. A test facility was designed and

assembled in which either of these scenarios could be investigated on a small scale. The test facility

contained a 12 litre helium vessel, together with a system of valves, sensors and high-speed data

acquisition. To carry out a test, the 12 litre vessel was filled with superfluid helium at 1.8 K. A fast-

acting valve was then used to open a large hole in the insulating vacuum to simulate a catastrophic leak,

or a very small hole to simulate a small leak. By monitoring the rise of pressure and temperature, and the

rate of change of mass of the vessel, the heat flux and venting rate could be calculated.

These results can be extrapolated directly to the AMS magnet, and have been used to qualify the

cryogenic system for flight on the Space Shuttle.

In addition to these investigations, tests have also been carried out on prototype burst discs.

Discs for protecting the vacuum tank have undergone vibration testing followed by controlled bursts.

These tests have shown that the discs are not affected by the levels of vibration encountered during a

launch. Further tests have been carried out on discs for protecting the helium vessel, which operate at

1.8 K. These discs have been shown to have extremely good leak tightness against superfluid helium.

Although the burst pressure is increased as a result of the low temperature, this increase has been found to

be predictable and reproducible. The next planned test is a vibration test under cryogenic conditions,

followed by a controlled burst.

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iv) Avionics In addition to extensive testing with the magnet, the CAB will undergo the full battery of space

qualification procedures for avionics listed in detailed in § 2.8. The UPS have an even more rigorous

series of tests at both the cell (currently in progress) and battery levels to ensure that they are safe and

reliable under all conditions.

The magnet has passed a special NASA Safety Review. Figure 2.24 shows the assembly of the

flux return coils.

Figure 2.24: Coil Assembly.

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2.1.6 References

[1] B. Blau, E. Ettlinger, S. Harrison et al., “The AMS02 superconducting magnet for astrophysical

research”, Gravitation and cosmology 5 (2000), Supplement pp. 1.

[2] B. Blau, S. Harrison, H. Hofer et al. “The superconducting magnet system of AMS-02 – a particle

physics detector to be operated on the International Space Station”, IEEE Transactions on

Applied Superconductivity 12 (2002) 349.

[3] G. Baccaglioni, B. Blau et al., “Production and Qualification of 40 km of Al-stabilized NbTi

Cable for the ATLAS Experiment at CERN”, IEEE Trans. On Applied Superconductivity, 12.1

(2002) 1215.

[4] L. Rossi, "Superconducting accelerators and detectors", Cryogenics 43 (2003) 281, see § 6.

[5] F. M. Ohlen, Astronomy and Astrophysics Supplement Series, 65.4 (1986) 607, and references

therein.

[6] S. M. Volz et al., “Cryogenic on-orbit performance of the NASA Cosmic Background Explorer

(COBE)”, SPIE Vol. 1340 Cryogenic Optical Systems and Instruments IV (1990).

[7] M. F. Kesseler et al., The ISO Handbook, Vol I “ISO - Mission & Satellite Overview”, ESA

SAI/2000-035/Dc, Ver. 2 (Nov 2003).

[8] M. J. DiPirro et al., “The transfer of superfluid helium in space”, Cryogenics 1994 vol. 34 ICEC

supplement.

[9] S. Harrison, E. Ettlinger, G. Kaiser, et al. “Cryogenic system for a large superconducting magnet

in space”, IEEE Transactions on Applied Superconductivity Vol. 13 pp. 1381-1384.

[10] A. Nekano, D. Petrac and C. Paine, “He II liquid/vapour phase separator for large dynamic range

operation”, Cryogenics Vol. 36, pp. 823-827.

[11] A. Kent, “Experimental low-temperature physics”, Macmillan, pp. 54-57.

[12] S. Breon et al., “Operation of a Sunpower M87 cryocooler in a magnetic field”, Cryocoolers 12,

Edited by Ron Ross, Jr., Kluwer Academic/Plenum Publishers, pp. 761-769, 2003.

[13] M. DiPirro, P. Shirron and J. Tuttle “Mass gauging and thermometry on the superfluid helium on-

orbit transfer flight demonstration”, Advances in Cryogenic Engineering Vol. 39, pp. 129-136,

1994.

[14] A. Mord and H. Snyder, “Self-driven cooling loop for a large superconducting magnet in space”,

Cryogenics Vol. 32, pp. 205-211, 1992.

[15] G. Kaiser et al., “Thermo-mechanical superfluid helium pumps for Alpha Magnetic Spectrometer

(AMS-02) mission”, Proceedings of the 19th International Cryogenic Engineering Conference,

pp. 523-526.

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-2+24+,&!8&,-;42)!41'&'4+2&*)+*4!2324+&,5'6(2+*4! &'-*'+*,(!-282(-*(6!,(!*+)!5'))!'(-!2(2&6<>! !H*(42! +12!

8'&+*432!5,52(+;5!*)!-2+2&5*(2-!7*+1!+12!FGH#C"!)*3*4,(!+&'4L2&!:<!52');&*(6!+12!+&'U24+,&<!*()*-2!+12!

5'6(2+I! +12! -2+24+2-! +&'()*+*,(! &'-*'+*,(! B%AD! 4'(!:2!;)2-! +,!-*)+*(6;*)1!:2+722(!8'&+*432)!,=! -*==2&2(+!

5'))2)I!3*L2!8,)*+&,()!'(-!8&,+,()>!!!

Page 62: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#VC!

%12!%A!81,+,()!'&2!-2+24+2-! *(!)+&'7! +;:2)I! =*332-!7*+1!'!W2XQY"! BZC[X"C[D!6')!5*\+;&2! B)22!

E*6;&2!">"]D!'(-!,82&'+2-!'+!/]CC!^>!!M*+1!'!8&,:':*3*+<!,=!':,;+!TC[!%A!81,+,()!'&2!8&,-;42-!*(!+12!"C!

55!+1*4L!=32242!'(-!-2+24+2-!:<!+12!)+&'7>!%12!8&*(4*8'3!,=!%AJ)!*)!92&<!7233!;(-2&)+,,-!'(-!+12<!'&2!

;)2-! *(! 3'&62! 8'&+*432! 81<)*4)! 2\82&*52(+)! BF%_FH!."0! '+! Q`ARI! N`AF#a!.V0! '+! J`HbD>! ! %12! (27!

41'332(62!*)!+,!,82&'+2!);41!'!3'&62!6')!-2+24+,&!)'=23<!'(-!&23*':3<!*(!)8'42>!

!20

mm

6 mm

Xe/CO2

Fiber

Radiator

!!

Figure 2.26: The operating principal of the AMS-02 Transition Radiation Detector.

!

2.2.1 Mechanical Structure

?(! +,+'3! V"Z! %AJ! 5,-;32)I! 2'41! 4,(+'*(*(6! /]! )+&'7)I! ,=! 32(6+1)! :2+722(! C>Z! '(-! "!5! '&2!

'&&'(62-! *(! "C! 3'<2&)! 2'41! 7*+1! "C!55! ,=! C>C]!6c45V! 8,3<8&,8<32(2c8,3<2+1<32(2! /C!-5! =*:2&! =32242>!!%12!3,72&!'(-!;882&!=,;&!3'<2&)!'&2!,&*2(+2-!8'&'3323!+,!+12!FGH#C"!5'6(2+*4!=*23-!71*32!+12!5*--32!/"!

3'<2&)!&;(!82&82(-*4;3'&!+,!8&,9*-2!VJ!+&'4L*(6>!!%12<!'&2!);88,&+2-!:<!'!4,(*4'3!,4+'6,(I!')!)1,7(!*(!

E*6;&2!">"dI!5'-2!,=!'3;5*(;5#1,(2<4,5:!7'33)!7*+1!4'&:,(#=*:2&!)L*()!'(-!:;3L12'-)>!!F!5241'(*4'3!

8&24*)*,(! ,=! :2++2&! +1'(! /CC!-5! '));&2)! 6')! 6'*(! 1,5,62(2*+<! :2++2&! +1'(! /[>! ! Y(! +12! ,;+)*-2! ,=! +12!4,(*4'3! ,4+'6,(! )+&;4+;&2! '! 6&*-! )+&;4+;&2! B)22! E*6;&2!">"TDI! :;*3+! ,;+! ,=! 4'&:,(! =*:2&! +;:2)I! 7*33! :2!

'++'412-!+,!);88,&+!+12!)2&9*42)!B6')!+;:2)I!N^!4':32)I!)*6('3!4':32)D>!

F! 4,;832-! 3,'-! '('3<)*)! ,=! +12! 2(+*&2! %AJ! )+&;4+;&2!.e0! 1')! :22(! 4'&&*2-! ,;+! :<! 52'()! ,=! '!

-2+'*32-!E*(*+2!`3252(+!Q'34;3'+*,(>!!F)!+12!&2);3+!,=!+12!5,-'3!'('3<)*)!+12!=*&)+!('+;&'3!2*62(#=&2f;2(4<!

+;&()!,;+!+,!:2!Te!NKI!':,92!+12!&2f;*&2-!TC!NK>!!E*6;&2!">"Z!)1,7)I!=,&!+12!5,)+!4&*+*4'3!-*&24+*,(!KI!+12!

&23'+*92! -*)83'4252(+)>! !^'&*,;)! 2\82&*52(+'3! +2)+)! B)22!E*6;&2!">"$D! 1'92!:22(!;)2-! +,! 92&*=<!5'+2&*'3!

8&,82&+*2)!'(-!'('3<+*4'3!4'34;3'+*,()!.T0>!!!

!

Page 63: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#V/

!!

Figure 2.27: The TRD Octagon Support Structure.

!

!!

Figure 2.28: TRD modal analysis results.

Page 64: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#V"!

!!

Figure 2.29: Vibration test stand loaded with a TRD straw module at RWTH-Aachen.

!

F)!)1,7(!*(!E*6;&2!">VCI!+12!/]!)+&'7)!*(!2'41!5,-;32!'&2!:;*3+!,;+!,=! +7,!,92&3'88*(6!L'8+,(!

)+&*8)!4,92&2-!7*+1!'3;5*(;5!'(-!6&'81*+2!,(!,(2!)*-2!'(-!8,3<2+1<32(2!,(!+12!:'4L)*-2!'(-!'&2!7,;(-!

:'4L#+,#:'4L!'(-!12'+!)2'32-!+,!=,&5!)+&'7!+;:2)!,=!">"!5!*(!32(6+1I!]!55!*(!-*'52+2&!'(-!d"!-5!7'33!+1*4L(2))>! !H*\+22(!)+&'7)!'&2!;)2-!+,!:;*3-!'!5,-;32>! !H*\!3,(6*+;-*('3!4'&:,(!)+*==2(2&)!'(-!'--*+*,('3!

4'&:,(! )+&*8)! &;((*(6! '4&,))! +12! 5,-;32! 292&<! /C!45! '));&2! 5241'(*4'3! &*6*-*+<! +,! 7*+1)+'(-! 3';(41!

9*:&'+*,()>! !%12!)+&'7)!'&2!43,)2-!7*+1!+7,!8,3<4'&:,('+2!2(-8*242)I!71*41!8&,9*-2! +12!6')#);883<!'(-!

42(+2&!+12!Q;#%2!4&*58#83;6)!.]0!+,!1,3-!+12!VC!-5!6,3-!83'+2-!+;(6)+2(!7*&2)!+2()*,(2-!7*+1!/!R>!!%12!8&24*)*,(!,=!+12!7*&2!8,)*+*,(*(6!7')!92&*=*2-!7*+1!'!1*61#&2),3;+*,(!4,58;+2&#+,5,6&'81<#)4'(!')!)1,7(!

*(!E*6;&2!">V/!'(-!7')!=,;(-!+,!:2!7*+1*(!VC!-5>!!

!

Figure 2.30: AMS-02 TRD module with 16 straw tubes.

!

!!

Figure 2.31: TRD Module Computer Tomography. The straw

walls and the central wires are clearly visible.

Page 65: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#VV

%12!,8+*5*K2-!FGH#C"!%AJ!-2)*6(!7*+1!'!-*'52+2&!,=!">"!5!'(-!T"eZ!)+&'7!+;:2)!'&&'(62-!*(!

"C!3'<2&)!72*61)!32))!+1'(!TCC!L6!B)22!%':32!">"D> !

!

Component Weight [kg]

A'-*'+,&! ]C!

H+&'7!%;:2!G,-;32)! Te!

Y4+'6,(! //e!

H;88,&+IH1*23-*(6!'(-!H2&9*42)! /CC!

W2XQY"! Te!

g')!H<)+25! ]V!

Q&'+2!`324+&,(*4)! TV!

Total 498

!

Table 2.2: Breakdown of the TRD weight.

!

!

2.2.2 Module Construction and Quality Control

%12!6')!+*61+(2))!,=!+12!)+&'7!5,-;32)!*)!+12!5,)+!4&*+*4'3!-2)*6(!*));2>!!%12!'9'*3':32!);883*2)!,=!

6')I!e$>T!L6!,=!W2!'(-!e>T!L6!,=!QY"I!7*33!1'92! +,! 3')+! =,&! +1&22!<2'&)!,=!,82&'+*,(>! !S)*(6!')!)+'(-'&-!

4,(-*+*,()!/!:'&!'(-!"$Z!PI!+1*)!4,&&2)8,(-)!+,!Ze"C!3!,=!W2!'(-!"TVC!3!,=!QY">!!%12!QY"!32'L!&'+2!=,&!

,(2!52+2&!,=!)+&'7+;:2!7')!52');&2-!+,!:2!C>"V!\!/C]!3!5:'&c)!7*+1!+12!%AJ!6')!W2XQY"!ZCX"C!5*\+;&2!

BE*6;&2!">V"D>! ! %1*)! 32'L! &'+2! *)! '++&*:;+2-! +,! -*==;)*,(! +1&,;61! +12! )+&'7! 7'33)>! ! ?+! 4,&&2)8,(-)! +,!

/>ZT!\!/CT!3!5:'&c)! 82&!5,-;32#52+2&! ,&! $>V!\!/C!V!3!5:'&c)! =,&! +12! =;33! %AJ! BTCC!5,-;32!52+2&)D>! ! F!

)*(632! 8,3<#4'&:,('+2! 2(-8*242! 1')! '!QY"! 32'L! &'+2! ,=! C>$!\!/C!T!3!5:'&c)I! =,&! '33! V"Zh"! 2(-8*242)! +1*)!

+,+'3)! +,! T>$!\!/C!V!3!5:'&c)>! ! H;55*(6I! +12! +,+'3! %AJ! QY"! 32'L! &'+2! ,=! />T!\!/C!"!3!5:'&c)! 7,;3-!

4,&&2)8,(-!+,!'!3,))!,=!QY"!,92&!V!<2'&)!,=!"Zd!3!,&!'!i)'=2+<!='4+,&j!,=!Z>Z!7*+1!&2)824+!+,!+12!QY"!);883<>!!

E':&*4'+2-!%AJ!5,-;32)!'&2!'4428+2-!*=!+12<!1'92!7*+1!'!QY"!)'=2+<!='4+,&!:2++2&!+1'(!e>!!%1*)!4'(!,(3<!

:2!'));&2-!:<!+2)+*(6!2'41!,=!+12!T"eZ!)+&'7)!*(-*9*-;'33<!:2=,&2!8&,-;4*(6!'!5,-;32!.d0>!!

F!)*(632!)+&'7!+2)+!)+'(-!BE*6;&2!">VVD!1')!:22(!-2923,82-!712&2!123*;5!*)!;)2-!+,!'41*292!=')+!

'(-!'44;&'+2!52');&252(+)>!!k2&!52+2&!,=!5,-;32I!'!123*;5!32'L!&'+2!,=!/C!\!/C#T!3!5:'&c) 4,&&2)8,(-)!+,!

+12!+'&62+!)'=2+<!='4+,&!,=!e!=,&!QY"!BE*6;&2!">VeD>!!F!)+&'7!*)!63;2-!6')!+*61+!'+!,(2!2(-!;)*(6!'!:&'))!83;6>!!

F!)+223!+;:2!*)!63;2-!+,!+12!,+12&!2(-I!)2&9*(6!')!'!6')!*(32+>!!%12!)+&'7!*)!83'42-!*()*-2!'(!2\+2&('3!9,3;52!

71*41! *)!5'-2!6')! +*61+!7*+1! '! 3*-! '(-!Y#&*(6>! !%1*)!9,3;52! *)! 4,((24+2-! +,! '! &2=2&2(42!9,3;52!9*'! '!

9'392! '(-! '! -*==2&2(+*'3! 8&2));&2! )2(),&>! ! %12! 9,3;52)! '&2! *(! +12&5'3! 4,(+'4+! '(-! +12! +2582&'+;&2! *)!

5,(*+,&2->! ! F=+2&! *()+'33'+*,(I! +12! 9'392! *)! ,82(2-! :&*2=3<! +,! 2f;'3*K2! +12! 8&2));&2! :2+722(! +12! +7,!

9,3;52)>! !%12(! +12!)+&'7!*)! =*332-!7*+1!123*;5!'+!'!8&2));&2!,=!">Z!:'&>! !N23*;5!6')!2(+2&)! +12!2\+2&('3!

9,3;52!-;2!+,!-*==;)*,(!+1&,;61!+12!)+&'7!7'33)!,&!-;2!+,!5'4&,)4,8*4! 32'L)>! !%12!-*==2&2(+*'3!8&2));&2!

*(4&2')2!*)!52');&2-!'(-!+12!32'L!&'+2!4'(!:2!-2+2&5*(2-!'=+2&!'!82&*,-!,=!T!5*(;+2)!BE*6;&2!">VTD>!

!

Page 66: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#Ve!

!!

Figure 2.32: Xe:CO2 leak rate measured with a mass spectrometer with three 1.3 m long straws.

!

!!

Figure 2.33: AMS-02 TRD single straw test stand.

!

Page 67: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#VT

F!-2+'*32-!-2)4&*8+*,(!,=!+12!)+&'7!5,-;32!8&,-;4+*,(!4'(!:2!=,;(-!*(!.ZI$0>!!F=+2&!=':&*4'+*,(!'33!

)+&'7!5,-;32)!;(-2&6,!+12!=,33,7*(6!+2)+)X!

+ k&2));&2!-&,8!+2)+X!%12!QY"!32'L!&'+2!,=!2'41!)+&'7!5,-;32!*)!52');&2-!:<!'!8&2));&2!-&,8!+2)+!'+!

/>d!:'&!*(!'!9'4;;5!92))23>!!F)!)1,7(!*(!E*6;&2!">V]I!+12!)'=2+<!='4+,&!'92&'62-!,92&!'33!5,-;32)!

)2324+2-!=,&!=3*61+!*)!d>$>!!%1*)!7,;3-!'33,7!;8!+,!"C!<2'&)!,=!,82&'+*,(!,(!+12!?HH>!!!

+ J'&L! 4;&&2(+X!%12! )+&'7)!5;)+! ,82&'+2!7*+1,;+! '(<! )*6(*=*4'(+! Bl! /!(FD! -'&L! 4;&&2(+! '+! '! 1*61!

9,3+'62!,=!/TCC!^!7*+1!F&XQY"!BZCX"CD>!!!

+ TTE2!6')!6'*(!1,5,62(2*+<! BE*6;&2!">VdDX! !%12!6')!6'*(!')! '! =;(4+*,(!,=! +12!8,)*+*,(!'3,(6! +12!

)+&'7)!*)!52');&2-!=,&!2'41!)+&'7!,=!+12!5,-;32!71*32!*+!*)!5,;(+2-!,(!'!8&24*)*,(!6&'(*+2!:3,4L!

+,! 2();&2! =3'+(2))>! ! %12! )+&'7! )*6('3)! '&2! 4';)2-! :<! 4,(92&+2-! T>$!L2^! 81,+,()! =&,5! '(! TTE2!

),;&42>!!%12!52');&2-!6')!6'*(!-*)82&)*,(!*)!&2f;*&2-!+,!:2!32))!+1'(!/>T![>!!

H8'42!f;'3*=*4'+*,(!+2)+)!1'92!:22(!4'&&*2-!,;+!=,&!2*61+!C>d!5!3,(6!)+&'7!5,-;32)>!!%12!5,-;32)!

;(-2&72(+!9*:&'+*,(!+2)+)!B'!C>T!6!)*(2!)7228!=,33,72-!:<!'!]>Z!6&5)!&'(-,5!+2)+!=,33,72-!'6'*(!:<!'!C>T!6!

)*(2!)7228DI!Z!4<432!+12&5,#9'4;;5!+2)+)!B)22!E*6;&2!">VZDI!:2+722(!!eC!!'(-!m]C!,QI!=,33,72-!'6'*(!:<!9*:&'+*,(!+2)+)>!!R,!)*6(*=*4'(+!41'(62)!*(!6')!+*61+(2))I!6')!6'*(!,&!2*62(#=&2f;2(4*2)!72&2!,:)2&92->!!!

0 1 2 3 4 5 6 7 8 9 10

20

40

60

80

100

120

140

160

leaky modules

flight modules

flight modules

Safety Factor CO

He

leak

rat

e (1

0-5

l mba

r/s/

m)

2, Vacuum

SF=3

SF=4

!!

Figure 2.34: Correlation between measured He and CO2 leak rates for modules that

underwent different processing methods. %12! ,82(! 4*&432)! &28&2)2(+!

5,-;32)!712&2! +12! *(-*9*-;'3! )+&'7)!72&2! +2)+2-!:2=,&2!'))25:3<I! =,&! +12!

5,-;32)!-2(,+2-!:<!43,)2-!4*&432)!+12<!72&2!(,+>!!R,+2!+1'+!,(3<!5,-;32)!

7*+1!'!)'=2+<!='4+,&!6&2'+2&!+1'(!e!'&2!;)2-!=,&!=3*61+>

Page 68: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#V]!

!!

Figure 2.35: Leak rate measurement of 3 straws, one acceptable,

two above the limit 10x10-5

l mbar/s/m (safety factor 4).

!

0

10

20

30

40

50

60

0 2 4 6 8 10 12

Entries

Mean

RMS

332

7.934

1.673

Safety Factor CO2, Vacuum

!!

Figure 2.36: Straw module production: safety factor CO2.

Mo

du

les

Page 69: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#Vd

0

5

10

15

20

25

30

35

40

0 0.5 1 1.5 2 2.5 3 3.5 4

Entries

Mean

RMS

316

1.456

0.5369

RMS Gasgain ArCO2 [%]

Figure 2.37: Straw module production status: Gas gain homogeneity

using Ar:CO2 (80:20) at a nominal gas gain of 3000.

Figure 2.38: TRD thermal vacuum test of 4 straw detector modules.

Mod

ule

s

!

Page 70: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#VZ!

2.2.3 TRD Electronics

%,! )28'&'+2! 8&,+,()! =&,5!8,)*+&,()I! 2+4I! '(,-2! )*6('3)! =&,5! *,(*K'+*,(! 3,))2)! '3,(2! 1'92! +,! :2!

-*)+*(6;*)12-!2==*4*2(+3<!=&,5!)*6('3)!4,(+'*(*(6!:,+1!+1*)!2(2&6<!-28,)*+!'(-!':),&:2-!%A!81,+,()!7*+1!'!

8;3)2!12*61+! &2'-,;+>! !%12! )*6('3)!,=! '33! )+&'7! +;:2)!'&2!-*6*+*K2-!'=+2&! '! )*6('3! =&,5! +12!62(2&'3!FGH!

+&*662&!'(-!=*3+2&2-!*(!+12!=*&)+!)+28!,=!-'+'!&2-;4+*,(>!!!Y(3<!6,,-!1*+)I!-2=*(2-!')!V"!':,92!+12!(,*)2!32923!

,&!':,;+!,(2! +2(+1! +12!)*6('3! 32=+!:<!'!)*(63<!41'&62-!5*(*5;5!*,(*K*(6!8'&+*432! BG?kDI!'&2!)2(+! +,! +12!

1*612&!32923)!)<)+25!,=!FGH!-'+'!'4f;*)*+*,(!BJFOD!)<)+25>!!!

%12! JFO! )<)+25! ,=! +12! %AJI! E*6;&2!">V$I! *)! -*9*-2-! *(+,! =&,(+! 2(-! 2324+&,(*4)I! 71*41! '&2!

5,;(+2-!-*&24+3<!,(! +12!-2+24+,&I! +7,!S#Q&'+2)I!71*41!1,)+! +12!JFO!'(-!)3,7!4,(+&,3!:,'&-)!'(-! +7,!

SkJ)!*(!71*41!+12!"Z!^JQ!);883*2-!=&,5!+12!kJH!*)!+&'()=,&52-!*(!+,!+12!3,7!9,3+'62)!(22-2-!:<!+12!

,+12&!%AJ!2324+&,(*4)>!!!

!

UPDUCrateFront End

Temp. meas.

to UGcrate

UFE

Trigger / DAQ

UTEUHVD

DataUDR2

UPSFE

JINF

UHVG

UPDfilter

Power / Data

HV

from / to

Ctrl PowerUBP

S90xxDC / DC

28VDC from PDS

Octagon

!!

Figure 2.39: Overview of the TRD data acquisition system.

!

F3+,62+12&!+1*)!2324+&,(*4)!4,();52)!32))!+1'(!/CC!M!B"CI!e"!'(-!VT!M!*(!+12!=&,(+!2(-I!S#Q&'+2)!

'(-!SkJ)D! +,!8,72&I! &2'-,;+! '(-! 4,(+&,3! +12!T"eZ!41'((23)!,=! +12!%AJ>! !%12! =&,(+! 2(-!2324+&,(*4)! *)!

-2923,82-I!:;*3+!'(-!+2)+2-!*(!F'412(>!!%12!S#Q&'+2!'(-!SkJ!'&2!U,*(+3<!-2923,82-!:<!F'412(I!P'&3)&;12!

'(-!G?%!'(-!7*33!:2!8&,-;42-!'(-!)8'42!f;'3*=*2-!'+!+12!Q1;(6#H1'(!?()+*+;+2!,=!H4*2(42!'(-!%241(,3,6<!

BQH?H%DI!%'*7'(>!!%12!9'&*,;)!)+28)!,=!+12!-2923,852(+!=&,5!=*&)+!8&,+,+<82)!+1&,;61!+12!f;'3*=*4'+*,(!,=!

+12!=3*61+!;(*+)!'&2!-2)4&*:2-!*(!n">Z>T>!!!

i) Front End electronics

`'41!,=! +12!V"Z!)+&'7!5,-;32)! *)!2f;*882-!7*+1!'!S%`!:,'&-!71*41!-*)+&*:;+2)! +12!N^! +,! +12!

)*6('3!7*&2)!'(-!:&*(6)!,;+! +12!)*6('3)!9*'!'!)1,&+!)*\+22(!=,3-!+7*)+2-!8'*&!4':32!+,!+12!=&,(+!2(-!:,'&-!

BSE`D>!!E,;&!)+&'7!5,-;32)!7*+1!+12*&!S%`!:,'&-)!'&2!4,5:*(2-!*(!'!6&,;8!,&!i+,72&j>!!`'41!,=!+12!Z"!

+,72&)!*)!);883*2-!:<!'!)28'&'+2!N^!41'((23!'(-!&2'-!,;+!:<!,(2!SE`!:,'&->!!%12!N^!=,&!'!+,72&!'&&*92)!

'+!'!SN^J!:,'&-!'(-!*)!-*)+&*:;+2-!+,!+12!=,;&!S%`!:,'&-)>!!

%12!SE`!:,'&-I!)1,7(!*(!E*6;&2!">eCI!*)!:')2-!,(!^F!'('3,6!5;3+*832\2&)!./C0>!!?+!*)!2f;*882-!

7*+1!'!)2&*'3!/"#:*+!'('3,6!+,!-*6*+'3!4,(92&+2&)!BFJQD!'(-!4,92&)!'!-<('5*4!&'(62!,=!eC!G?k)!B'+!'!6')!

6'*(!,=!VCCCD>!!%12!&2'-,;+!+*52I!*(43;-*(6!+12!-*6*+*K'+*,(!,=!+12!]e!4,((24+2-!41'((23)I!*)!Zd!o)>!!!

Page 71: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#V$

!!

Figure 2.40: TRD Frontend readout board, UFE.

!

%12! 5,;(+*(6! ,=! +12! =&,(+! 2(-! 2324+&,(*4)! -*&24+3<! ,(! +12! ,4+'6,(I! *()*-2! +12! 5;3+*#3'<2&!

*();3'+*,(!BG_?DI!'));&2)!'(!2324+&*4'3!)1*23-*(6!71*41!L228)!+12!(,*)2!32923!:23,7!"!FJQ!41'((23)>!!%12!

-*))*8'+2-!12'+!L228)!+12!52'(!%AJ!+2582&'+;&2!:2+722(!!/T!'(-!mVT!,Q>!!F33!+12!=&,(+!2(-!:,'&-)!1'92!:22(!)8'42#f;'3*=*2-!7*+1!+12!)+&'7+;:2!5,-;32)>!!?(!'--*+*,(!+,!9*:&'+*,(!'(-!+12&5'3!9'4;;5!+2)+)I!+12!

2324+&,5'6(2+*4! *(+2&=2&2(42! 7')! 52');&2-! 7*+1! =,;&! />e!5! 5,-;32)! 5,;(+2-! *(! '! 4'&:,(#

=*:2&c'3;5*(;5#1,(2<4,5:!:,\!B')!+12!%AJ!,4+'6,(D!7&'882-!*(!G_?!=,*3>!%1*)!*(43;-2-!1*61!=&2f;2(4<!

25*))*,(! '(-! );)428+*:*3*+<! )+;-*2)>! ! E*6;&2!">e/! )1,7)! '(! '4428+':32! %AJ! =&,(+2(-! &2'-,;+! 25*))*,(!

)824+&;5!'=+2&!'88&,8&*'+2!)1*23-*(6>!!!

%2582&'+;&2!52');&252(+)!*()*-2!+12!,4+'6,(!'&2!5'-2!7*+1!-*6*+'3!+2582&'+;&2!)2(),&)!BJ'33')!

JH/ZH"CDI!71*41!'&2!'++'412-!+,!+12!Sg#Q&'+2!B)22!n!">">T>*D>!!!

!

!!

Figure 2.41: TRD Frontend electromagnetic emission test results.

!

! !

Page 72: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#eC!

ii) U-Crate

`'41!,=! +12!+7,!S#Q&'+2)!4,(+'*()! +12!-'+'!'4f;*)*+*,(!)<)+25I!+12!-*)+&*:;+*,(!,=!3,7!'(-!1*61!

9,3+'62!+,!+12!=&,(+!2(-!2324+&,(*4)!'(-!+12!4,(+&,3!,=!'33!:,'&-)!'(-!9,3+'62)!=,&!1'3=!+12!%AJ>!!%12!=&,(+!

2(-!2324+&,(*4)!*)!4,((24+2-!+,!)*\!:,'&-)!BSJA"D!71*41!8&,9*-2!+12!=*&)+!32923!,=!-'+'!&2-;4+*,(>!!%1*)!

+<82! ,=! :,'&-! 4,()*)+)! ,=! '! -;'3! &2-;(-'(+! 4,55,(! -*6*+'3! 8'&+! BQJkD! '(-! '! -2+24+,&! -282(-'(+! 8'&+!

BJJkD>!!!

!

DSP

PROM

Mem.

DSP

PROM

Mem.

Sequencer Sequencer

!2.0V+2.0V{4x

Tri

gg

erB

usy

Tri

gg

erB

usy

Dat

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ISO

Dat

aC

om

man

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and

s/

CLK

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r

Reg

iste

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ISO

DAC

4x4x

CLK

SSF SSF

UFE

Digital Power+3.3V

JIN FUPSFE UP D

DACDAC

UPSFE

GateArray

GateArray

AM

Sw

ire

AM

Sw

ire

JIN F

CDP_a CDP_b

DDP

UFE UFE UFE UFE UFE UFE

Ctrl

!!

Figure 2.42: Design of the TRD data reduction board, UDR2.

!

%12!QJk!4,55;(*4'+2)!7*+1!+12!1*612&!32923)!,=!+12!FGH!JFO!)<)+25!9*'!'!1*61!)822-!)2&*'3!

3*(LI!FGH7*&2I!+1&,;61!+12!p?RE!:,'&->!!!%12!JJk!*)!'(!*(+2&='42!:2+722(!+12!4,55,(!-*6*+'3!8'&+!,=!+12!

SJA"!'(-!+12!SE`!:,'&-)>!!N2&2!+12!)*6('3)!=,&!+12!&2'-,;+!)2f;2(42!'&2!+&'()=2&&2-!+,!+12!SE`!:,'&-!

9*'!-24,;83*(6!41*8)!B?HYD!+,!'-U;)+!+12!-*==2&2(+!9,3+'62!32923)!,=!+12!QJk!BmV>V!^JQD!'(-!+12!=&,(+!2(-!

Bq">C!^JQD>!!F!-*6*+'3!+,!'('3,6!4,(92&+2&!BJFQD!=,&!4'3*:&'+*,(!8&,42-;&2)!*)!'3),!*(43;-2->!!E,&!2'41!

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);:+&'4+*,(!'(-!K2&,!);88&2))*,(!'(-!'++'412)!'!62,6&'81*4'3!'--&2))>!!a24';)2!,=!+12!'&&'(6252(+!,=!+12!

&2'-,;+!*(!e!3'<2&!+,72&)I!+<8*4'33<!,(3<!,(2!SE`!82&!SJA"!7*33!1'92!9'3*-!1*+)>!!

Y+12&!:,'&-)!*(!2'41!,=!+12!S#Q&'+2)!62(2&'+2!'(-!4,(+&,3!)+':32!3,7!'(-!1*61!9,3+'62)!=,&!+12!e/!

+,72&)>! ! %1*)! *)! '&&'(62-! *(! +1&22! 8,72&! 6&,;8)I! 2'41! 4,(+'*(*(6! /V! ,&! /e! +,72&)I! +7,! SJA")I! ,(2!

SkHE`I!=,&!+12!3,7!9,3+'62!4,(+&,3!'(-!+7,!SN^g!=,&!+12!1*61!9,3+'62!62(2&'+*,(>!%12!SkHE`!4,()*)+)!

,=! )292(! -;'3! &2-;(-'(+! 3*(2'&! &26;3'+,&)! B_AD!71*41! )+':*3*K2! +12! 9,3+'62)! -23*92&2-! +,! +12! SE`! '(-!

8&,+24+!'6'*()+!,92&!4;&&2(+!'(-!;(-2&!9,3+'62>!!`'41!_A!4'(!:2!)7*+412-!,==!9*'!'!4,55'(->!!%12!SN^g!

:,'&-)!4,(+'*(!)292(!-;'3!&2-;(-'(+!Q,4L&,=+#M'3+,(!2329'+,&)!*(!71*41!/"C!^JQ!*)!5;3+*83*2-!*(!'!/]!

Page 73: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#e/

)+'62!-*,-2!4'8'4*+,&!4')4'-2>!!Q,(+&,3!*)!8&,9*-2-!:<!'(!GN^/CC!'883*4'+*,(!)824*=*4!*(+26&'+2-!4*&4;*+!

BFH?QDI!-2923,82-!:<!_2Q&,<!A2)2'&41!H<)+25)!)824*=*4'33<!=,&!FGH>!!!

%12!p?RE!:,'&-!'3),!)2&92)!')!'!4,55'(-!'(-!5,(*+,&*(6!*(+2&='42! +,! +12!SkHE`I!SN^g!'(-!

+12!SkJ!;)*(6!]!)2&*'3!:;))2)>!!!

!

! iii) UPD

%12!SkJ!1,)+)!'(!*(8;+c,;+8;+!=*3+2&!BH$C//aD!'+!+12!"Z^JQ!=22-!*(8;+!)*-2I!'!-,;:32!&2-;(-'(+!

4,(+&,332&!:,'&-!BH$C//FSD!'(-!JQ#JQ!4,(92&+2&)>!!Y(2!H$CTV!62(2&'+2)!mV>V!^JQ!=,&!'33!-*6*+'3!8'&+)!

*(!+12!S4&'+2!'(-!+12!H$C//FS>!!%1&22!H$CeZ!62(2&'+2!q">]!^JQ!=,&!+12!=&,(+2(-!'(-!+12!JJk>!!%1&22!

H$CT]!62(2&'+2!m/"C!^JQ!')!*(8;+!9,3+'62!+,!+12!Q,4L&,=+#M'3+,(!2329'+,&!'(-!mT>C!^JQ!=,&!+12!GN^!

4,(+&,332&>! !F33! +12!JQ#JQ!4,(92&+2&)! '&2! -;'3! &2-;(-'(+! ;(*+)>! ! %12! '4+*92! ;(*+! 4'(! *)! 4,(+&,332-! '(-!

5,(*+,&2-!:<!+12!H$C//FS>!!!

2.2.4 Thermal Model

%12!+12&5'3!)+':*3*+<!,=!+12!%AJ!*)!2))2(+*'3!=,&!+12!82&=,&5'(42!,=!+12!-2+24+,&!')!+2582&'+;&2!

9'&*'+*,()!41'(62!+12!6')!-2()*+<!'(-!12(42!+12!6')!6'*(>!!%,!L228!+12)2!9'&*'+*,()!:23,7!+12!=27!82&42(+!

32923I! 4,58'&':32! +,! +12!5,-;32! +,!5,-;32! *(+2&#4'3*:&'+*,(!;(42&+'*(+*2)!-*)4;))2-!:23,7I! +2582&'+;&2!

6&'-*2(+)!7*+1*(! +12!%AJ!)1,;3-!(,+!2\422-!//!,Q>! !%12! +12&5'3!4,(+&,3! )+;-<!1')!:22(!82&=,&52-!:<!YNa!H<)+25I!a&252(I!g2&5'(<>!

%,!L228! +12! )8'+*'3! '(-! +258,&'3! ,&:*+! +2582&'+;&2! 6&'-*2(+! :23,7!/!,Q! +12!%AJ!7*33! :2! =;33<!4,92&2-! *(!5;3+*#3'<2&#*();3'+*,(! BG_?DI! *(43;-*(6! +12! =&,(+! 2(-! 2324+&,(*4)>! !F! +12&5'3! )*5;3'+*,(! =,&!

,&:*+!8'&'52+2&)!71*41!7*33!6*92!+12!1*612)+!%AJ!+2582&'+;&2!)7*(6!')!)1,7(!*(!E*6;&2!">eV!8&,92)!+12!

2==24+*92(2))!,=!+1*)!'88&,'41>!!R,(2+1232))I!+1*)!7*33!:2!:'4L2-!;8!:<!'!=;33!)4'32!+12&5'3!9'4;;5!+2)+>!!

!

!

Figure 2.43: TRD thermal simulation.

2.2.5 Gas System

%12!62(2&'3!3'<,;+!,=!+12!FGH#C"!%AJ!6')!)<)+25!*)!)1,7(!*(!E*6;&2!">ee>!!a,\!H!1,3-)!+12!W2!

'(-!QY"!)+,&'62!92))23)!7*+1!);==*4*2(+!6')!=,&!+12!V#T!<2'&!FGH#C"!5*))*,(!7*+1!'!)'=2+<!5'&6*(!,=!=,;&>!!

?+! 8&,9*-2)!a,\!Q!7*+1!8&25*\2-!6')! =&,5!'! 3*5*+2-! +&'()=2&!9,3;52! Br/! 3*+2&D!;(-2&! 4,58;+2&! 4,(+&,3!

-'*3<>! ! a,\!Q! 4,(+'*()! 8;58)! '(-! 9'392)! +,! 4,(+&,3! +12! 6')! 4*&4;3'+*,(>! ! ?+! '3),!5,(*+,&)! 6')! f;'3*+<>!

G'(*=,3-)! -*)+&*:;+2! +12! 6')! +,! +12! T"eZ! 8&,8,&+*,('3! 7*&2! +;:2)I! 71*41! '&2! '&&'(62-! *(! e/! 8'&'3323!

)2652(+)>!!!

!

Page 74: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#e"!

Figure 2.44: AMS-02 TRD gas system general layout.

a,\2)! H! '(-! Q! '&2! 5,;(+2-! :21*(-! '! -2:&*)! )1*23-! ,(! +12! SHH! ,(! +12! 7'L2! )*-2! ,=! FGH!

BE*6;&2!">eTD>! %12! 5'(*=,3-)! '&2! 5,;(+2-! ,(! +12! ;882&! 8'&+)! ,=! +12! &'5! '(-! 7'L2! )*-2)! ,=! +12! %AJ!

,4+'6,(I! *()*-2! *+)! +12&5'3! 2(43,);&2>! ! %,! L228! +12! ),32(,*-! 9'392)! *(!a,\2)! H! '(-!Q! ':,92! T!,QI! +12!'))25:3<!*)!2(43,)2-!*(!G_?!'(-!+12!9'392!:3,4L)!'&2!=*++2-!7*+1!12'+2&)>!!N2'+2&)!'&2!'3),!5,;(+2-!,(!+12!

6')!+'(L)!+,!L228!+125!':,92!+12!4&*+*4'3!+2582&'+;&2)!,=!W2!B/d!,Q!D!'(-!QY"!BV/!,QDI!),!+1'+!+12!'5,;(+!,=!6')!&25'*(*(6!4'(!:2!52');&2-!:<!+12!8&2));&2>!!!

!

!!

Figure 2.45: Location of TRD Gas system elements

%12! )4125'+*4! =,&! a,\!H! *)! )1,7(! *(! E*6;&2!">e]>! ! %7,! )+,&'62! 92))23)! )+,&2! +12! \2(,(! '(-!

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Page 75: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#eV

!!

Figure 2.46: Schematics of Box S, Box C, and one of the 41 Manifold segments.!

Page 76: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#ee!

_2'L#:2=,&2#:;&)+!92))23)!2();&2!)'=2+<!*(!+12!292(+!,=!1*61!+2582&'+;&2)!4';)*(6!,92&!8&2));&2!*(!

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i) TRD Gas system electronics

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%12!SgkJ!4,(+'*()!'!=*3+2&!=,&!+12!"Z!^JQ!*(8;+!=&,5!+12!kJHI!'!4,(+&,3!:,'&-!'(-!+12!JQ#JQ!

4,(92&+2&)!(242))'&<!+,!8&,9*-2!9,3+'62!'(-!4;&&2(+!+,!,82&'+2!9'392)I!8;58)!'(-!,+12&!8'&+)!,=!+12!%AJ!

6')!)<)+25!'(-!+12!4,55'(-!2324+&,(*4)>!!!

F33!4,(+&,3!'(-!5,(*+,&!2324+&,(*4)!,82&'+2!*(!+12!)+&'<!=*23-!=,&5!+12!FGH!5'6(2+!,=!r/ZC!g>!!!

%12! 2(+*&2! %AJ! 6')! )<)+25! 2324+&,(*4)! *)! -;'3! &2-;(-'(+! '+! +12! :,'&-! 32923>! ! %12! )<)+25! 4'(!

4,(+*(;2! +,! ,82&'+2! 8&,82&3<! 292(! *(! +12! 292(+! ,=! 5;3+*832! ='*3;&2)! *(! -*==2&2(+! +<82)! ,=! :,'&-)>! ! %,!

*583252(+! +1*)! =2'+;&2I! =,&! 292&<! :,'&-! *(! ,82&'+*,(I! +12!hot board,! '! )+'(-:<! ;(*+I! +12! cold board,! *)!

8&,9*-2-!BE*6;&2!">eZD>!

Page 77: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#eT

%12! 2(6*(22&*(6! 5,-;32)! ,=! +12! 4,(+&,3! 2324+&,(*4)! BE*6;&2!">e$D! 1'92! :22(! +1,&,;613<! +2)+2-!

7*+1!+12!'4+;'3!8'&+)!,=!+12!6')!)<)+25>!!!

!

!!

Figure 2.47: TRD gas system command and control architecture.

!

UG-Crate

UGPD

TRD GAS

Box C Box S

ma

nif

old

s

TRD

CAN-BUS

120VDC28VDC

HV safety signal to U crate

Ctrl & monitor signals

Power

Gas

1553 LRDL (NASA Avionics)

USCM UGBC UGFVUGBS

UGPS

module

JMDC Monitoring &

control computer

Ctrl

Filter PDS

DC-DC

converters

Page 78: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#e]!

!!

Figure 2.48: Boards in the TRD gas system electronics crate, UG-Crate.

Figure 2.49: TRD gas system electronics boards.

!

ii) Box S Tests

Q,58,(2(+!+2)+)!1'92!:22(!4'&&*2-!,;+!,92&!+12!8')+!+1&22!<2'&)!,(!+12!)8'42!f;'3*=*2-!9'392)I!+12!

8&2));&2! )2(),&)! '(-! '33! +12! *(3*(2! 6')! =*++*(6)! B=3,7! &2)+&*4+,&)I! =*3+2&)I! :;==2&! 9,3;52)! '(-!5241'(*4)!

=*++*(6)D>!!%12!9'392)!'(-!)2(),&)!1'92!:22(!+2)+2-!'(-!,82&'+*,(!92&*=*2-!,92&!+12!,82&'+*(6!+2582&'+;&2!

&'(62! BC! +,! meC!,QD! '(-! +12! );&9*9'3! &'(62! B!"C! +,! m]T!,QD>! ! F33! +2)+)! 72&2! 4'&&*2-! ,;+! '+! 5'\*5;5!2\824+2-!,82&'+*(6!8&2));&2>!!!

Page 79: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#ed

%7,! 9*:&'+*,(! +2)+)! 1'92! :22(! 4'&&*2-! ,;+! ,(! +12! )+,&'62! )<)+25! 2(6*(22&*(6!5,-23! '+! `R`FI!

Q'))'44*'I! ?+'3<!7*+1! +12! ?RER!A,5'! 6&,;8! +,! 2();&2! +12!5241'(*4'3! *(+26&*+<! ,=! +12! )<)+25! '(-! +12!

=;(4+*,('3*+<!,=!+12!4,58,(2(+)!'=+2&!3';(41!')!7233!')!+,!9'3*-'+2!+12!=*(*+2!23252(+!4'34;3'+*,(>!!!

%12! )<)+25! ')! +2)+2-! *)! )1,7(! *(! E*6;&2!">TC>! ! %12! +2)+! 8&,42-;&2!7')! +,! 82&=,&5! =*&)+! '! )*(2!

)7228I!=,33,72-!:<!'!&'(-,5!9*:&'+*,(!'(-!'!=*('3!)*(2!)7228I!'33!'3,(6!+12!)'52!4,,&-*('+2!'\*)>!!%1*)!

8&,42-;&2!7')!4'&&*2-!,;+!=*92!+*52)X!,(42!'3,(6!+12!u!'\*)!'(-!+7*42!2'41!'3,(6!W!'(-!b>!!F=+2&!2'41!

)2&*2)! ,=! +1&22! 9*:&'+*,()I! '! =;(4+*,('3! +2)+! 7')! 82&=,&52-! ,(! +12! 6')! 4*&4;*+)! +,! 5'L2! );&2! '33! +12!

5241'(*4'3! 23252(+)! )+*33! =;(4+*,(>! ! ?(!2'41!4')2I! 4,58'&*),(!,=! +12! )*(2! )7228!4'&&*2-!,;+!:2=,&2!'(-!

'=+2&! +12!&'(-,5!9*:&'+*,(!)1,72-! +12&2!1'-!:22(!(,!41'(62! *(! +12!2*62(=&2f;2(4*2)!,=! +12!)<)+25!'(-!

12(42!(,!41'(62! *(! )+&;4+;&'3! *(+26&*+<>!%12! 3,72)+! 2*62(=&2f;2(4<!7')! =,;(-! +,!:2!':,92!d/!NKI!7233!':,92!+12!&'(62!,=!9*:&'+*,()!2\82&*2(42-!-;&*(6!3';(41!BE*6;&2!">T/D!.//0>!

S)*(6!'(!2(6*(22&*(6!5,-23!,=!+12!4,(+&,3!2324+&,(*4)I!'33!4,58,(2(+)!,=!a,\!H!72&2!);442))=;33<!

,82&'+2-!;(-2&!';+,(,5,;)!4,58;+2&!4,(+&,3!-;&*(6!)292&'3!5*\*(6!4<432)!BE*6;&2!">T"D>!!!

!!

Figure 2.50: Box S engineering prototype and test fixture (yellow) mounted on slip table.

71 Hz!!

Page 80: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#eZ!

Figure 2.51: Vibration testing of the Box S mechanics. The figure in the upper left shows the

results of finite element modeling and the figure on the upper right the locations of the

accelerometers during the test. The upper half of the graph shows response to the

excitations in the lower half during an x-axis sine sweep.

!

C

B

G

x

y z

C

B

G

Frequency (Hz)

0 20 100 200 50

Phase

Response

Page 81: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#e$

!Figure 2.52: Fill cycle using electronics under computer control for Box S. Pressure measurements

show the buildup of gas while mixing and then a release simulating filling.

iii) Box C Tests

%12!4*&4;3'+*,(!)<)+25!4,(+'*()! +7,!4*&4;3'+*,(!8;58)!7*+1!'44,58'(<*(6!9'392)! *()*-2!'!)+223!

92))23>!!%12!=;(4+*,(*(6!,=!+12!8;58)!,92&!+12!=;33!+2582&'+;&2!&'(62!1')!:22(!+2)+2-!*(!'!4,3-!:,\>!!%12<!

=;(4+*,(!7*+1!'!)3*61+!B/C[D!41'(62!*(!4;&&2(+>!%12!9'392)!1'92!'3),!:22(!+2)+2-!,92&!+12!2(+*&2!&'(62!'(-!

'&2!=,;(-!+,!7,&L!-,7(!+,!v/T!,Q!BE*6;&2!">TVDI!7233!:23,7!+12!5*(*5'3!,82&'+*,('3!+2582&'+;&2!,=!C!,Q>!!!

%12!5,(*+,&!+;:2!'))25:3<!1')!'3),!:22(!+2)+2-!:<!5'L*(6!6'*(!52');&252(+)!7*+1!F&XQY"!'(-!

W2XQY"!BZCX"CD>!!%12!52');&2-!6')!8'&'52+2&)!5'+41!+12!L(,7(!9'3;2)!7233!'(-!+12!5,(*+,&!+;:2!)<)+25!

82&=,&5)!&23*':3<>!%12!)8*&,52+2&I!71*41!*)!;)2-!+,!52');&2!+12!QY"!4,(+2(+!:<!52');&*(6!),;(-!923,4*+<I!

1')!:22(!+2582&'+;&2!4<432-!,92&!+12!);&9*9'3!&'(62!5'(<!+*52)!'(-!4,(+*(;2)!+,!7,&L>!

%12!2(6*(22&*(6!5,-23!,=!a,\!Q!1')!:22(!'))25:32-!7*+1!'33! *(+2&('3!4,58,(2(+)!83'((2-!=,&!

=3*61+I!E*6;&2!">Te>!!F!+2)+!'&+*432!=,&!+12!43,)2#,;+!723-)!1')!:22(!5'-2!'(-!+12!=*&)+!723-!+2)+!82&=,&52->!

E;(4+*,('3!+2)+)!,=!+12!92))23!1'92!:22(!4'&&*2-!,;+!'(-!'33!+12!*(+2&('3!4,58,(2(+)!82&=,&5!7233>!!F!=*&)+!

+2582&'+;&2! 4<432! +2)+! ,=! +12! 2(6*(22&*(6! 92&)*,(! ,=! +12! 92))23! 1')! :22(! 4'&&*2-! ,;+! );442))=;33<>! ! F)!

2\824+2-I!+12!8;58!-&'7)!),5271'+!5,&2!4;&&2(+!'+!3,7!+2582&'+;&2)>!?(!+1*)!+2)+!+12!9'392)!4,(+*(;2-!+,!

,82&'+2!'+!v"C!,Q!'5:*2(+>!!

iv) Manifold tests

%12! 9'392)! '(-! 8&2));&2! )2(),&)! 1'92! :22(! );442))=;33<! f;'3*=*2-! ,92&! +12*&! +2582&'+;&2! &'(62!

'(-! '! 5'(*=,3-! '))25:3<! 7')! 9*:&'+*,(! +2)+2-! '+! AM%N>! ! ! M*+1! +12! '--*+*,(! ,=! />V!55! ^'4,=3;\!

)1*23-*(6I!+12<!1'92!);442))=;33<!8'))2-!'!=;(4+*,('3!+2)+!*(!+12!"CC!g!5'6(2+*4!=*23-!71*41!4,&&2)8,(-!+,!

+12*&!,82&'+*,('3!2(9*&,(52(+>!

A2)2+!

"C[!QY"!

ZC[!W2!

M'*+!

A232')2!

Page 82: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#TC!

%12!5'(*=,3-!'))25:3*2)!1'92!:22(!+2)+2-!;)*(6!+12!2(6*(22&*(6!5,-23!,=!2324+&,(*4)!4,(+&,332-!

')!=,&!=3*61+>!!`'41!9'392!*(!'!9'392!)2+!7')!4<432-!;(-2&!/!:'&!,=!'&6,(!'(-!+12!8&2));&2!)2(),&)!&2'-!,;+!

'=+2&!2'41!4<432>!!?(!'33!4')2)I!+12!9'392)!'(-!8&2));&2!)2(),&)!=;(4+*,(2-!')!2\824+2->!!!

!

!

Figure 2.53: Histogram of temperatures at which the valve failed

to open (minimum operating temperature is 0 ,C).

! !!

Figure 2.54: Left - Engineering model of Box C vessel with pump visible at in the opening.

Right - Vessel with end cap in place and gas feedthrough.

Page 83: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#T/

2.2.6 TRD Prototype Performance

%,!92&*=<! +12!8&,+,(!&2U24+*,(!8,72&!,=! +12!FGH#C"!%AJ!-2)*6(!'! =;33!"C! 3'<2&!8&,+,+<82!7')!

:;*3+!7*+1! eC!5,-;32)! ,=! eC! 45! *(! 32(6+1! '&&'(62-! *(! +7,! '-U'42(+! +,72&)I! 2f;*882-!7*+1!^F! '('3,6!

5;3+*832\2&!:')2-!=&,(+2(-!2324+&,(*4)>!!?(!E*6;&2!">TT!+12!6')!8'(23!);883<*(6!)*\!41'*()!4'(!'3),!:2!)22(>!!!

!

!

Figure 2.55: AMS-02 TRD 20 layer prototype.

%1*)!)2+;8!7')!;)2-!*(!+12!Q`AR!%$I!Wd!'(-!N]!:2'5!3*(2)!+,!&24,&-!V!5*33*,(!+&'4L)!./V0>!!%12!

8'&+*432! +&*662&! 7*+1! )4*(+*33'+,&! 8'(23)! '(-! +1&2)1,3-! ,&! -*==2&2(+*'3! Q2&2(L,9! 4,;(+2&)! '33,72-! +12!

)2324+*,(! ,=! 2324+&,()I! 5;,()! '(-! 8*,()! ;8! +,! /CC!g2^! '(-! 8&,+,()! ;8! +,! "TC!g2^>! ! %12! -'+'!

8&28&,42))*(6! 92&*=*2-! +12! 3,7! (,*)2! 32923! 7*+1! 82-2)+'3! 7*-+1)! :23,7! "!FJQ! 41'((23)! '(-! '(! *(+2&#

4'3*:&'+*,(!8&24*)*,(!:23,7!"[!'41*29':32!7*+1!TCCC!+&'4L)>!!%12!6')!6'*(#-2()*+<!4,&&23'+*,(!'+!/edC!^!

B6')! 6'*(! TCCCD!7')! -2+2&5*(2-! +,! :2!.gcg!w!!T>T!.' c' >! ! %12! ':),3;+2! 2(2&6<! )4'32!7')! 4'3*:&'+2-!7*+1!'(!TTE2!),;&42>!!!

GQ!)*5;3'+*,(!)+;-*2)!'&2!;)2-! +,!,8+*5*K2! +12!-2+24+,&!-2)*6(>! !%12<!'&2!:')2-!,(! +12!8&,92(!

g2'(+V!./e0!-2+24+,&!)*5;3'+*,(!8'4L'62!7*+1!'--*+*,('3!4,-2!./T0!+,!*(43;-2!%A!81,+,(!62(2&'+*,(!'(-!

':),&8+*,(!./]0!'(-!+,!*58&,92!+12!)*5;3'+*,(!,=!-`c-W!_'(-';#=3;4+;'+*,()!*(!+1*(!6')!3'<2&)!./d0>!!%12!

+2)+!:2'5!-'+'!'&2!;)2-!+,!+;(2!+12!GQ!8'&'52+2&)!+,!-2)4&*:2!,;&!-2+24+,&!&2)8,()2>!!E*6;&2!">T]!)1,7)!

+12!2(2&6<!)824+&'!52');&2-!=,&!'33!7*&2)!*(!*),3'+2-!)*(632!+&'4L!292(+)>!!%12!8&,+,(!)824+&;5!)1,7)!+12!

2\824+2-!_'(-';!=3;4+;'+*,()>!!E,&!2324+&,()!'(!2(1'(4252(+!-;2!+,!+12!+&'()*+*,(!&'-*'+*,(!4,58,(2(+!*)!

432'&3<!9*)*:32!':,92!]!L2^>!!!

%,!'('3<K2!+12!+2)+!:2'5!&2);3+)I!8&,+,()!'&2!)28'&'+2-!=&,5!2324+&,()!7*+1!'!3*L23*1,,-!'36,&*+15>!!

%12!2(2&6<!)824+&'!*(!E*6;&2!">T]!'&2!;)2-!')!8&,:':*3*+<!-2()*+*2)! DBEp >!!M*+1!2'41!2(2&6<!-28,)*+! iE !*(!

n !+;:2)!,(!+12!&24,()+&;4+2-!+&'4LI!(,&5'3*K2-!8&,:':*3*+<!8&,-;4+)!'&2!-2=*(2-!')! n nipepe EpP 12

/II DB >!!

Page 84: 2004 Ams Nim Paper Draft

AMS-02/TRD

!"#T"!

M*+1! '! 3*L23*1,,-! -2=*(2-! ')X! DcB pee PPPL %2 !+12! 8&,+,(! &2U24+*,(! ='4+,&! *)! -2+2&5*(2-! ')! +12! *(92&)2!

8&,+,(!)2324+*,(!2==*4*2(4<!7*+1!'!3*L23*1,,-!4;+!)2+!=,&!'(!2324+&,(!2==*4*2(4<!,=!$C[>!!E,&!8&,+,(!:2'5!

2(2&6*2)!:2+722(!/T!'(-!"TC!g2^!+12!8&,+,(!&2U24+*,(!*)!7233!':,92!/CC!')!)1,7(!*(!E*6;&2!">Td>!!!

!

!!

Figure 2.56: Clean single track energy spectra.

!!

Figure 2.57: AMS-02 TRD proton rejection.

Page 85: 2004 Ams Nim Paper Draft

AMS-02/TRD

! "#TV

2.2.7 References

./0! ?>!E&'(LI!^>!g*(K:;&6I!p>!k1<)>!9!B/$eTD!VTV>!

."0! F%_FH!%JA!TI!^,3>"I!Q`ARc_NQQc$d#/d>!

.V0! N`AF#aI!J`Hb#kAQ!CCcCeI!"CCC>!

.e0! xFGH#C"!H+&;4+;&'3!^2&*=*4'+*,(!k3'(xI!pHQ#"Zd$"I!A29>!Q>!

.T0! Space Qualification of the AMS-02 Transition Radiation Detector, +,!:2!);:5*++2-!+,!R?G!F>!

.]0! A>!a,4L!et al.I!R?G!F!336!B/$$VD!/"Z>!

.d0! Construction of Straw Detector Modules for the AMS-02 Transition Radiation DetectorI! +,! :2!

);:5*++2-!+,!R?G!F>

.Z0! %1>!P*&(!et al.,!Status of AMS-TRD-Straw modulesI!Q,(=>!k&,4>!%AJ)! =,&! +12!V&-!5*332((*;5I!

a'&*!"CCVI!);:>!R?G!F>!

.$0! %1>!P*&(!et al.I!E&')4'+*!k1<)*4)!H2&*2)!^,3>!XXV B"CC/DI!/]/#/d">!

./C0! E>!N';32&I!The AMS-02 Transition Radiation Detector for the International Space StationI!Q,(=>!

k&,4>!?```!RHH!"CCVI!);:>!?```!RH>!

.//0! F>a'&+,3,(*I!The AMS-02 TRD gas Control System;!R?G!F518!B"CCVD!/eV>!

./"0 Q>g'&6*;3, et al.I!The Mechanical Design of a Gas Supply and Mixing System for AMS-02;!k&,4>!

?FQ#CV#p>k>!//s!Te+1!?(+>!F)+&,(';+*4'!Q,(=>!H28+25:2&!"CCVI!a&252(I!g2&5'(<>!!

./V0! Performance of the AMS-02 Transition Radiation DetectorI!+,!:2!);:5*++2-!+,!R?G!F>!!

./e0! A>!a&;(!et al>I!g`FR%>!Q`AR!JJc``cZe#/!Bg2'(+!V>"/!A29*)2-!/$ZdD>!

./T0! ^>!`6,&<+4129I!^>!H'923*29I!H>p>!F83*(I!R;43>!?()+&>!'(-!G2+1>!F!453!B"CCCD!Ve]>!

./]0! G>!Q12&&<I!k1<)>!A29>!J!10!B/$deD!VT$e>!

./d0! ^>!`&5*3,9'!et al.,!R?G!F!145!B/$ddD!TTT>!

Page 86: 2004 Ams Nim Paper Draft

AMS-02/Tracker

!"#$%!

!"# $%&%'()*+,-'./,*&'(!)*+#,-!+./.012!&3405(3!6-7!849! :'(!;.39:!4<</.04:.12! .2!9<40(!1;! :'(!'.='!<3(0.9.12!9./.012!

:(0'21/1=>!?(@(/1<(?! ;13! <19.:.12!A(49B3(A(2:9! .2! 400(/(34:13! (C<(3.A(2:9!6"7D! ! &'(! '.='!A1?B/43.:>E!

/18!@1/:4=(!/(@(/9!FG-,,!HIE!42?!=49#;3((!1<(34:.12!1;!:'(!?(@.0(!.9!8(//!9B.:(?!:1!1<(34:.12!.2!9<40(D!!&'(!

-JJK! 9'B::/(! :(9:! ;/.=':! ?(A129:34:(?! L1:'! :'(! 9B00(99;B/! 4?4<:4:.12! 1;! :'(! :(0'21/1=>! :1! :'(! 9<40(!

([email protected](2:!42?!:'(!;(49.L./.:>!1;!/43=(!43(4!?(:(0:139D!!!

&'(!)*+#,"!+./.012!&3405(3!?(9.=2!42?!0129:3B0:.12!.9!B2?(3!:'(!1@(34//!3(9<129.L./.:>!1;!MNON#

P(3B=.4D! ! &'(! 499(AL/>! 1;! :'(! 9./.012! /4??(39E! 8'.0'! 3(<3(9(2:9! 4! 9BL9:42:.4/! <43:! 1;! :'(! 0129:3B0:.12!

(;;13:E!.9!<(3;13A(?!4:!MNON#P(3B=.4E!Q2.@(39.:>!1;!R(2(@4!42?!4:!42!M:4/.42!.2?B9:3.4/!3(9(430'!;40./.:>-!

1<(34:.2=! B2?(3! 42! )+M! 012:340:D! ! P(39122(/! 1;! :'(! Q2.@(39.:>! 1;! SB0'43(9:! 42?! 1;! M++#SB0'43(9:!

012:3.LB:(?!:1!:'(!9./.012!/4??(3!499(AL/>D!!&'(!&3405(3!A(0'42.04/!9B<<13:!49!8(//!49!:'(!&3405(3!/49(3!

4/.=2A(2:! 9>9:(A! 43(! ?(9.=2(?! 42?! LB./:! L>! )40'(2D! ! &'(! T)U! (/(0:312.09! 42?! <18(3! 9>9:(A9! 8(3(!

?(@(/1<(?!4:!:'(!Q2.@(39.:>!1;!R(2(@4!42?!MNON#P(3B=.4!.2!01//4L134:.12!8.:'!*M&!42?!V+M+&!42?!8.//!

L(! ;4L3.04:(?! 4:!V+M+&D! ! &'(! 12/.2(! ?4:4! 3(?B0:.12! 91;:843(! .9! ?(@(/1<(?! 4:!*12<(//.(3D! ! &'(!&3405(3!

&'(3A4/!V12:31/!+>9:(A!.9!?(9.=2(?!42?!LB./:!L>!NWX!.2!01//4L134:.12!8.:'! :'(!Q2.@(39.:>!1;!R(2(@4E!

+B2!Y4:#9(2!Q2.@(39.:>E!RB42=Z'1BE!42?!MNON#P(3B=.4D!!!!

+./.012! A.031#9:3.<! 9(29139! 8(3(! 13.=.24//>! ?(@(/1<(?! ;13! @(3:(C! ?(:(0:139! .2! 01//.?.2=#L(4A!

(C<(3.A(2:9! .2!13?(3! :1!<31@.?(!4! ;(8!'.='!<3(0.9.12!<19.:.12!A(49B3(A(2:9! 2(43! :'(! .2:(340:.12!<1.2:D!!

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Page 93: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 94: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 95: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 96: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 97: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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AMS-02/Tracker

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Page 99: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 100: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 101: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 102: 2004 Ams Nim Paper Draft

AMS-02/Tracker

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Page 103: 2004 Ams Nim Paper Draft

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6$7! uDSD!S.35E!P310D!P'>9D!+10D!)!CJ!F-J$-I!K_%D!

6^7! RD!)AL319.!et al.E!NB0/D!M29:3D!42?!*(:'D!)#C0!F-JJ$I!J_D!!!

6_7! *D!P4B/BZZ.E!NB0/D!M29:3D!42?!*(:'D!)!J[#!F",,-I!^_D!

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6-,7! RD!)AL319.E!NB0/D!M29:3D!42?!*(:'1?!)!J#5!F-JJJI!"-$D!

6--7! uD!H42?(2'.3:ZE!e.2!M2;3431:!W49(3!P19.:.129#p12:31//#+>9:(A!;o3!?49!)*+!eC<(3.A(2:E!",,-E!

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9(99.12!hRE!5*F",,-I!"-J_D!!!

6-%7! qD!q4//34;;!(:!4/DE!P310!_:'!M2:(324:.124/!V12;(3(20(!12!)?@420(?!&(0'21/1=>!42?!P43:.0/(!

P'>9.09!FMV)&PP#_IE!M#H.//4!h/A1!V1A1E!*D!S4312(!(:!4/D!Fe?9DIE!q13/?!+0.(2:.;.0E!+.2=4<13(E!

M+SN!JK-#"]K#-K,#$E!F",,"I!-%JD!!!

6-$7! HD!H(::(3/(E!+./.Z.BA!)/.=2A(2:!+(2913(2!;o3!?(2!)*+#,"!&3405(3!4B;!?(3!M++E!",,-E!

T.</1A43L(.:E!Xq&l#)40'(2D!!!

6-^7! )D!h9:4<:0'1B5!(:!4/DE!J!*4>!",,-E!V*+!N1:(!",,-c,$]E!V*+!z!VeXND!

6-_7! uD!)/0434Z!(:!4/DE!M/!NB1@1!V.A(2:1!#!H1/D!--"!)E!00!F",,,I!-]"$D!

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AMS-02/TOF

! "#$%

2.4 Time of Flight (TOF) &'()'*! +,-#."/! ()0! 1'20! 34! 56'7)(! 8195:! ;<'*('66=(3>;! ?>3@'A0! ()0! 4=;(! (>'770>! 43>! <)=>70A!

?=>('<60;! =*A! <3*@0>(0A! ?)3(3*;/! ;060<('3*/! =(! ()0! (>'770>! 60@06/! 34! ?=>('<60;! B'()'*! ()0! 2='*! +,-!

=<<0?(=*<0/! 20=;C>020*(! 34! ()0! ?=>('<60! @063<'(D! '*<6CA'*7! ()0! A';<>'2'*=('3*! E0(B00*! C?B=>A! =*A!

A3B*B=>A!73'*7!?=>('<60;!=*A!=!20=;C>020*(!34!()0!=E;36C(0!<)=>70!B)'<)!<32?6020*(;!()3;0!2=A0!'*!

()0!3()0>!A0(0<(3>;F!!1)0!195!;D;(02!34!()0!+,-#."!A0(0<(3>!';!E0'*7!EC'6(!=(!()0!GH5H!I=E3>=(3>'0;!'*!

J3637*=F! G(! ';! E=;0A! 3*! ?>0@'3C;! B066#0;(=E6';)0A! (0<)*'KC0;!L%M! =E60! (3! >0=<)! =! ?>0<';'3*! '*! ()0! ('20!

>0;36C('3*!34!%..!?;F!!1)0!A0;'7*!43663B;!()0!0N?0>'0*<0!7='*0A!B'()!()0!+,-#.%!A0(0<(3>!L"M/!23A'4'0A!

(3!(=O0!'*(3!=<<3C*(!()0!A'440>0*(!<3*A'('3*;!'*!+,-#."/!'*!?=>('<C6=>/!()0!;(>3*70>!;(>=D!2=7*0('<!4'06A!=(!

()0!?)3(32C6('?6'0>!(CE0;!8P,1;:F!!

1)0! 70320(>'<=6! =<<0?(=*<0! 34! ()0! 195/! =*A! <3*;0KC0*(6D! +,-#."! 43>! <)=>70A! ?=>('<60;/! ';!

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1)';! 2=(<)0;! ()0! =<<0?(=*<0! 34! ()0! ;'6'<3*! (>=<O0>! B'()'*! ()0! 2=7*0(F! ! +;! ;)3B*! '*! 5'7C>0!"F%! =*A!

5'7C>0!"F$S/! ()0! 195! ;D;(02! ';! <32?3;0A! 34! 43C>! >3C7)6D! <'><C6=>! ?6=*0;! 34! %"!<2! B'A0! ;<'*('66=(3>!

?=AA60;/!3*0!?='>!34!?6=*0;!=E3@0!()0!2=7*0(/!()0!C??0>!195/!=*A!3*0!?='>!E063B/!()0!63B0>!195F!!T=<)!

?6=*0!)=;!=!;0*;'('@0!=>0=!34!%F"!2"!=*A!B'()'*!3*0!?6=*0!()0!?=AA60;!=>0!3@0>6=??0A!ED!.FU!<2!(3!=@3'A!

70320(>'<=6!'*044'<'0*<'0;F!!53>!044'<'0*(!E=<O7>3C*A!>0V0<('3*!=*A!(3!='A!()0!3446'*0!=*=6D;';/!()0!?=AA60;!

'*!()0!(B3!=AV=<0*(!?6=*0;!=>0!?0>?0*A'<C6=>F!!T=<)!?=AA60!';!'*;(>C20*(0A!B'()!(B3!P,1;!=(!0=<)!0*AF!!!

1)0!195!;D;(02!?>3@'A0;!=!@0>D!4=;(!=*A!>06'=E60!>0;?3*;0!(3!()0!0*0>7D!63;;!34!<)=>70A!?=>('<60;/!

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C;0A!=;!()0!>040>0*<0!('20!43>!()0!0@0*(!8;00!=6;3!Y!"F$:F!!1)0!3@0>6=??'*7!=*A!<>3;;0A!?=AA60!70320(>D!34!

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=*A!=!7=(0!34!U.!*;F!!!

1)0! >0;36C('3*! '*! ()0! ('20! 34! 46'7)(! *00A0A! (3! ;=(';4D! ()0! ?)D;'<;! >0KC'>020*(;! ';! %".!?;F! 1)0!

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(3!>0=<)!()';!>0;36C('3*F!!W3B*B=>A!73'*7!<)=>70A!?=>('<60;!=>0!A';('*7C';)0A!4>32!C?B=>A!73'*7!=(!()0!

60@06!34!%.SF!!!

1)0! ;D;(02!20=;C>0;! ()0! 0*0>7D! 63;;! ED! =! <)=>70A! ?=>('<60! 8(3! 4'>;(! 3>A0>! ?>3?3>('3*=6! (3! ()0!

;KC=>0!34!()0!?=>('<60!<)=>70:!B'()!=!>0;36C('3*!;C44'<'0*(!(3!A';('*7C';)!*C<60'!C?!(3!<)=>70!\!Z!".F!1=O'*7!

'*(3! =<<3C*(! ()0! =((0*C=('3*! =63*7! ()0! <3C*(0>;/! =*A! ()0! *00A! (3! )=@0! =! 733A! 20=;C>020*(! 34! ;'*76D!

<)=>70!?=>('<60;/!=!AD*=2'<!>=*70!34!23>0!()=*!%./...!'*!()0!20=;C>020*(!34!()0!?C6;0!)0'7)(!';!>0KC'>0AF!!

&'()'*!+,-#."/!()';!20=;C>020*(!<32?6020*(;!()3;0!2=A0!ED!()0!;'6'<3*!(>=<O0>!=*A!]G^_F!!!

1)0!195!;D;(02!200(;!()0!>0KC'>020*(;!'2?3;0A!ED!()0!*00A!(3!3?0>=(0!;0@0>=6!D0=>;!3*!3>E'(F!!

T=<)!?=AA60!';!0*<=;0A!'*!=!20<)=*'<=66D!>3EC;(!=*A!6'7)(#('7)(!<3@0>!=*A!()0!;C??3>(!;(>C<(C>0!<3*43>2;!

(3!()0!H+-+!;?0<'4'<=('3*;!<3*<0>*'*7!>0;';(=*<0!(3!63=A!=*A!@'E>=('3*;F!!1)0!060<(>3*'<;!B'();(=*A;!()0!

)'7)6D! '3*'R'*7! 63B! T=>()! 3>E'(! 0*@'>3*20*(F! !,3>03@0>! ()0! ;D;(02! 7C=>=*(00;! >0AC*A=*<D/! B'()! (B3!

P,1;!3*!0=<)!0*A!34!()0!?=AA60;!=*A!A3CE60!>0AC*A=*(!060<(>3*'<;F!!1)0!;D;(02!<=*!3?0>=(0!'*!@=<CC2!

3@0>! ()0! (02?0>=(C>0! >=*70! `".! (3!aU.!,^b!)=;!=!B0'7)(!34! 60;;! ()=*!"$.!O7!=*A!=!?3B0>!<3*;C2?('3*/!'*<6CA'*7!=66!060<(>3*'<;/!34!60;;!()=*!%c.!&F!-D;(02!<32?3*0*(;!)=@0!E00*!KC=6'4'0A!43>!C;0!'*!;?=<0!=*A!

)=@0!E00*!(0;(0A!B'()!?=>('<60!E0=2;F!!!

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AMS-02/TOF

!"#$"!

Bracket

Bracket

UPPER TOF

LOWER TOF

Honeycomb

Honeycomb

Cover

Cover

Cover

Covers

Covers

PMTs, paddles

PMTs, paddles

PMTs, paddles

PMTs, paddles

!!

Figure 2.89: Exploded view of the AMS-02 time of flight (TOF) system.

!

!

2.4.1 Construction of the TOF

G*! =AA'('3*! (3! ()0! >0KC'>020*(;! (3! 3?0>=(0! >06'=E6D! '*! ;?=<0! 43>! d#U! D0=>;! =*A! (3!B'();(=*A! ()0!

6=C*<)!=*A!6=*A'*7!63=A;!B)0*!+,-#."!';!'*!()0!;)C((60/!()0!195!<3C*(0>;!2C;(!3?0>=(0!'*!()0!;(>=D!4'06A!

34!()0!+,-#."!<>D32=7*0(F!!5'7C>0!"FS.!;)3B;!()0!2=7*0('<!4'06A!'*!()0!>07'3*!34!()0!195!?6=*0;/!B)'<)!

>=*70;!C?!(3!d!OeF!!1)0!C;0!34!2=7*0('<!;)'06A'*7!';!?>0<6CA0A!E0<=C;0!34!()0!6=>70!B0'7)(!>0KC'>0A!=*A!

()0!'*AC<0A!43><0;!3*!()0!=;;02E6DF! !^3*;0KC0*(6D/!=!()3>3C7)!'*@0;('7=('3*!;060<(0A!=!P,1!B)'<)!<=*!

3?0>=(0!C*A0>! ()0;0!<3*A'('3*;!f! ()0!_=2=2=(;C!]USQg!f!?>3@'A0A! ()0!P,1!=N';! ';! =6'7*0A!B'()'*!QU!

A07>00;!34! ()0! 4'06A!A'>0<('3*F! !1)';!)=;!E00*!=!?>'2=>D!A0;'7*!<3*;'A0>=('3*! '*! ()0! <3*;(>C<('3*!34! ()0!

195!;D;(02F!!!

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! "#$d

!!

Figure 2.90: Magnetic field at the level of the TOF planes. PMT

locations are indicated by the dashed circles.

+;!;)3B*!'*!5'7C>0!"FS%/!0=<)!34!()0!43C>!?6=*0;!';!<32?3;0A!34!$!3>!%.!?=AA60;F!!1)0!?=AA60;!=>0!

%!<2!()'<O!=*A!%%c!(3!%dQ!<2!63*7F!!1)0!0A70!?=AA60;!=>0!(>=?0R3'A=6!B'()!=!B'A()!34!%$FU!(3!"gFS!<2F!!

1)0!3()0>!?=AA60;!=>0!%"!<2!B'A0! >0<(=*760;F! !+;! ;)3B*! '*!5'7C>0!"FS"/!0=<)!?=AA60! ';!<32?3;0A!34!=!

<0*(>=6!;0<('3*!34!TIhTH!Th#"..!;<'*('66=(3>!=AV3'*0A!=(!0=<)!0*A!ED!<60=>!<C>@0A!3>!E0*(!6'7)(!7C'A0;!C?!

(3!%U!<2!63*7!(3!=6'7*!()0!P,1!<3>>0<(6D!'*!()0!2=7*0('<!4'06A!=*A!(B3!3>!()>00!<3*'<=6!6'7)(!7C'A0;!B)'<)!

=A'=E=('<=66D!2=(<)!()0!P,1!?)3(3<=()3A0!=>0=;F!!!

+;!;)3B*!'*!5'7C>0!"F$S/!()0!?=AA60;!43>!()0!C??0>!863B0>:!?6=*0!?='>!=>0!23C*(0A!3*!()0!(>=<O0>!

;'A0!34!=!%.!<2!8U!<2:!()'<O!)3*0D<32E!?=*06F!!^=>E3*!4'E0>!0*<63;C>0;!8.FU!=*A!.Fc!22!()'<O:!?>3@'A0!

;C??3>(!=*A!6'7)(#('7)(*0;;F! !-?0<'=6!<=>0! ';! (=O0*!(3!=663B!()0;0!@36C20;!(3!@0*(!AC>'*7!6'4(!344F! !1)0;0!

<3@0>;!=6;3!;C>>3C*A!=*A!;C??3>(!()0!P,1;!=*A!=((=<)0A!060<(>3*'<;F!!1)0!C??0>!=*A!63B0>!195!=>0!0=<)!

23C*(0A!@'=!E>=<O0(;!(3!()0!i--/!)3B0@0>!=;!()0!;(>C<(C>=6!>0KC'>020*(;!=*A!'*(0>4=<0;!43>!()0!C??0>!=*A!

63B0>! =;;02E6'0;! =>0! A'440>0*(/! ()0!23C*('*7! E>=<O0(;! =>0! A'440>0*(F! ! 5'7C>0!"FSd! ;)3B;! 4'*'(0! 06020*(!

23A06! <=6<C6=('3*! 34! ()0! A';?6=<020*(;! 43>! ()0! 4'>;(!23A0! 34! ()0! 63B0>! 195/!B)'<)/! =(! U.!_R/! ';!B066!

=E3@0!()0!4>0KC0*<'0;!34!()0!;)C((60!0*7'*0;F!!!

!

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AMS-02/TOF

!"#$Q!

!!

!!

Figure 2.91: Top view of the design and flight paddles during an assembly

test of the upper (left) and lower (right) TOF.

Page 117: 2004 Ams Nim Paper Draft

AMS-02/TOF

! "#$U

!

!!

Figure 2.92: Design of a TOF paddle and photograph of an assembled paddle

after thermal vacuum and electrostatic discharge tests.

!

!

Figure 2.93: Finite element modeling of the lower TOF displacements (in meters).!

Page 118: 2004 Ams Nim Paper Draft

AMS-02/TOF

!"#$g!

2.4.2 PMT

G*! (3(=6/! ()0! 195! A0(0<(3>! ';! '*;(>C20*(0A! B'()! %QQ! _=2=2=(;C! ]USQg! P,1;F! ! 1)0D! =>0!

<D6'*A>'<=66D!;)=?0A/! jj4'*0!20;)kk!P,1;!=*A!B0>0!<)3;0*!43>! ()0'>!733A!?0>43>2=*<0! '*!)'7)!2=7*0('<!

4'06AF!!1)0!P,1!)=;!=!E'=6O=6'!?)3(3<=()3A0/!=!E3>3;'6'<=(0!76=;;!B'*A3B!=*A!%g!E'=6O=6'!AD*3A0;F!!1)0!

;?0<(>=6! >0;?3*;0!>=*70;! 4>32!d..! (3!g..!*2!B'()!=!2=N'2C2!>0;?3*;0!=(!Q".!*2!8<3>>0;?3*A'*7! (3!=!

KC=*(C2! 044'<'0*<D! 34! =E3C(! ".[:/! B)'<)! 2=(<)0;! ()0! ;<'*('66=(3>! 3C(?C(F! ! 1D?'<=6! <)=>=<(0>';('<;! =(!

"...!l! =*A! "U!,^! =>0m! =! <=()3A0! 6C2'*3C;! ;0*;'('@'(D! 8"$Ugn:! 34! Z$.!o+p62b! =*! =*3A0! 6C2'*3C;!;0*;'('@'(D!8"$Ugn:!34!Z$.!o+p62b!=!7='*!34!%.g!(3!%.cb!=*!=*3A0!A=>O!<C>>0*(!34!ZUF.!*+b!(>=*;'(!('20!34!

ZcF"!*;F!!!

1)0!0440<(;!34!2=7*0('<!4'06A!3*!()';!P,1!B0>0!(0;(0A!=(!GH5H!J3637*=!LdMF!1)0!20=;C>020*(;!

B0>0!2=A0!C;'*7!=! >0A! 6'7)(!02'(('*7!A'3A0! 8ITW:!3?0>=(0A! ()>3C7)!=!^+,+^!23AC60F!1)0! 6'7)(!B=;!

7C'A0A!(3!()0!P,1!ED!(B3!3?('<=6!4'E0>;F!1)0!P,1!B=;!?6=<0A!'*;'A0!()0!?360;!34!=!Q!Oe!060<(>32=7*0(!

3*!=!(>=*;6=('3*!=*A!>3(=('3*!;(=*AF!!1)0!P,1!>0;?3*;0!B=;!20=;C>0A!43>!A'440>0*(!2=7*0('<!4'06A!@=6C0;!

=*A!=*760;F!!!

5'7C>0!"FSQ! ;)3B;! ()0! >06=('@0! ?C6;0! )0'7)(! 43>! A'440>0*(! @=6C0;! 34! ()0! 4'06A! '*(0*;'(D! =*A! 43>!

A'440>0*(! P,1! 3>'0*(=('3*;! '*;'A0! ()0! 2=7*0('<! 4'06A/! B'()! >0;?0<(! (3! R0>3! 4'06AF! ! 53>! =*760;! =E3@0!

QU!A07>00;/!()0!>0;?3*;0!34!()0!P,1;!A07>=A0;!>=?'A6D!'4!()0!4'06A!';!7>0=(0>!()=*!.FU!(3!%!OeF!!1)0!('20!

>0;?3*;0!B=;!20=;C>0A!ED! 46=;)'*7!E3()! ()0! 4'*0!20;)!P,1!=*A! =! >040>0*<0!_=2=2=(;C!]US..!P,1!

B'()!()0!;=20!ITW!?C6;0F!!5'7C>0!"FSU!;)3B;!()0!2=7*0('<!4'06A!0440<(!3*!()0!('20!20=;C>020*(F!+7='*/!=!

;0>'3C;!A0(0>'3>=('3*!34!()0!('20!>0;36C('3*!3<<C>;!B)0*!()0!(CE0!';!3?0>=(0A!=(!=*760;!=E3@0!QU!A07>00;/!

'*A0?0*A0*(6D!34!()0!=??6'0A!2=7*0('<!4'06AF!!1)0!(>=*;'(!('20!@=>'=('3*!34!()0!P,1;!B=;!20=;C>0A!(3!E0!

=E3C(!"!?;pl36(!LQMF!!!

!

!!

Figure 2.94: Effect of magnetic field on the charge response of R5946 PMTs.

!

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AMS-02/TOF

! "#$c

!!

Figure 2.95: Effect of magnetic field on the time response of R5946 PMTs.

13! ;060<(! ()0! 46'7)(! P,1;/! ()0D! )=@0! =66! E00*! <)=>=<(0>'R0A! C;'*7! ()0! 20()3A;! A0@063?0A! 43>!

+,-#.%!LUMF!!+;!=*!0N=2?60/!5'7C>0!"FSg!;)3B;!()0!(02?0>=(C>0!A0?0*A0*<0!34!()0!7='*!43>!(B3!P,1;/!

20=;C>0A!C*A0>!@=<CC2F! !+4(0>!<=6'E>=('3*/! ()0!3?0>=('*7!_l!43>!0=<)! (CE0! (3!0KC=6'R0! ()0!>0;?3*;0! (3!

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!

Page 120: 2004 Ams Nim Paper Draft

AMS-02/TOF

!"#$$!

0

-50

50

100

150

200

250

300

-50 0 50 100 150 200 250 300

T (

Time (hours)

C)Pu

lse

heig

ht (m

V)

AIR VACUUM

PMT 5893

PMT 5975

!!

Figure 2.96: PMT response during thermal vacuum testing (upper)

and the applied temperature variation (lower).

!!

Figure 2.97: PMT in housing with HV divider.

Page 121: 2004 Ams Nim Paper Draft

AMS-02/TOF

! "#$S

2.4.3 Trigger and Electronics of the TOF and ACC

&'()'*!+,-#."/!()0!195!;D;(02!?>3@'A0;!()0!4'>;(!'*A'<=('3*!()=(!=!<)=>70A!?=>('<60!)=;!?=;;0A!

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!

!!

Figure 2.98: Fast trigger efficiency for different ions as a function of threshold applied on the

energy loss measured by a single counter at each end or both ends, in units of MIP.

Page 122: 2004 Ams Nim Paper Draft

AMS-02/TOF

!"#S.!

!!

Figure 2.99: TOF and ACC electronics scheme.

!

1)0! 060<(>3*'<;! ';! '2?6020*(0A! '*! 43C>! ;CE;D;(02;b! 0=<)! ';! <32?3;0A! 34! =! ;(=*A=>A! +,-!

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@=<CC2!<=;0!<3*'<=6!46=*70!8;00!Y!"FU:F!!!

!

Detector

S!crate

SFET

SFET

SFET

SFET

SDR

SFEA

SFEC

SFEC

/mon

+5.6 V!5.6 V

+5.6 V+3.3 V

SPT

analog part

digital part

(cold half)(hot half)

!!

Figure 2.100: TOF and ACC electronics power distribution.

Page 123: 2004 Ams Nim Paper Draft

AMS-02/TOF

! "#S%

1)0!-5T^!E3=>A;!A'7'('R0!()0!=*3A0!=*A!AD*3A0!;'7*=6;!4>32!0=<)!P,1!C;'*7!=!<'><C'(!A0@063?0A!

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!

2.4.4 Space qualification

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!

Page 124: 2004 Ams Nim Paper Draft

AMS-02/TOF

!"#S"!

-40 -30 -20 -10 0 10 20 30 40 50 60

160

180

200

220

240

260

280

300 Y = AX2 + BX + C

PMT 5893

A=(–0.5 ± 0.2) x10-2

A=(–0.6 ± 0.2) x10-2

B=–0.68 ± 0.09

B=–0.70 ± 0.07PMT 5975

T ( C)

Puls

e he

ight

(mV)

!!

Figure 2.101: PMT response as a function of the temperature in vacuum.

Dark current vs PMT temperature

1

10

10 2

-40 -30 -20 -10 0 10 20 30 40 50 60T ( C)

Dark

Cur

rent

(ua)

PMT ZH5974 at HV=1520 V

1

10

10 2

-40 -30 -20 -10 0 10 20 30 40 50 60T ( C)o

o

Dark

Cur

rent

(ua)

PMT ZH5915 at HV=1865 V

!!

Figure 2.102: PMT dark current as a function of the temperature.

Page 125: 2004 Ams Nim Paper Draft

AMS-02/TOF

! "#Sd

2.4.5 Beam test results

1)0!195!<3C*(0>;!B0>0!(0;(0A!'*!'3*!E0=2;!=(!^T]H!'*!".."!=*A!=7='*!'*!"..dF!1)0!E0=2;!B0>0!

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(=>70(/! B'()'*! A'440>0*(! 2320*(C2! ?0>! *C<603*! B'*A3B;! C;'*7! ()0! _$! ;060<('3*! 6'*0F! ! G*! ".."! ()0!

>0;?3*;0! 34! ()0! <3C*(0>;!B0>0! <32?=>0A! (3! 3*0!34! ()0!+,-#.%! <3C*(0>;F! ! G*! "..d/! 43C>! <3C*(0>;!B'()!

A'440>0*(!<3*4'7C>=('3*;!34!()0!6'7)(!7C'A0;!B0>0!(0;(0AF!!P>06'2'*=>D!>0;C6(;!=>0!?>0;0*(0A!E063BF!!!

5'7C>0!"F%.d! ;)3B;! ()0! (B3! <3C*(0>;! (0;(0A! '*! "..d! 8^"! =*A! ^d:! B)'<)! =>0! ()0! (B3! 23;(!

<)=660*7'*7!6'7)(!7C'A0;!B'()!^d!E0*(!=*A!^"!(B';(0A!=*A!E0*(F!!^3C*(0>;!^%!=*A!^Q/!E043>0!=*A!=4(0>!^"!

=*A!^d!'*!()0!E0=2!6'*0/!)=@0!;(>='7)(!6'7)(!7C'A0;F!!!

1)0! '3*! <)=>70! ';!B066!20=;C>0A! ED! =66! <3C*(0>;F! ! 1)0!20=;C>020*(! 4>32! ()0! =*3A0! ;'7*=6! 34!

<3C*(0>! ^"/! '*! ?>'*<'?60! ()0! B3>;(! 3*0/! ';! ;)3B*! '*! 5'7C>0!"F%.QF! ! 1)0! <)=>70! >0;36C('3*! 34! ^"! 43>!

A'440>0*(!'3*;!';!;)3B*!'*!5'7C>0!"F%.U!43>!E3()!()0!=*3A0!=*A!AD*3A0!;'7*=6;!;C220A!4>32!(B3!P,1;F!!

,0=;C>020*(;!4>32!()0!".."!(0;(!E0=2!>C*!=>0!<32?=>0A!B'()!()3;0!34!()0!+,-#."!]G^_!06020*(!()=(!

B=;!=6;3!'*!()0!E0=2!6'*0!'*!5'7C>0!"F%.gF!

1)0!('20!34!46'7)(!20=;C>020*(!E0(B00*!()0!^"!=*A!^d!<3C*(0>;! ';!;)3B*!'*!5'7C>0!"F%.c!=;!=!

4C*<('3*! 34! ()0! ?=>('<60! <)=>70F! ! +;! ()0!20=;C>020*(! '*! +,-#."!B'66! E0! A3*0!B'()! 43C>! '*A0?0*A0*(!

20=;C>020*(;/!()0!('20!>0;36C('3*!B)'<)!<=*!E0!'*40>>0A!';!34!()0!3>A0>!34!%d.!?;!43>!=!,GPF!

!

Counter C2:bent andtwisted lightguides.

Counter C3:bent lightguides.

173416291322

16171704

1489

1172

1624

110

110

191

119

1010

98

120

120

!!

Figure 2.103: The C2 and C3 counters with bent and twisted light guides,

tested in an ion beam at the CERN SPS in 2003.

Page 126: 2004 Ams Nim Paper Draft

AMS-02/TOF

!"#SQ!

!!

Figure2.104: The square root of the integrated charge measured with anodes and

dynodes show peaks corresponding to different beam particles. Peak

“2p” is produced by two singly charged particles crossing the

scintillator in time.

!

Page 127: 2004 Ams Nim Paper Draft

AMS-02/TOF

! "#SU

02

0.1

4

0.2

6

0.3

8

0.4

10

0.5

Z C2DR

Z C2AR

! Z! Z

0 2 4 6 8 10 12

12

0

0.1

0.2

0.3

0.4

P1 0.4805E!01

P1

0.1393E!02

P2

0.8314E!01

0.2630E!01

0.1467E!02

P2

0.6542E!03

0.2116E!01 0.6830E!03

!!

Figure 2.105: C2 charge resolution as a function of the particle charge

for anode (above) and dynode (below) signals.

Page 128: 2004 Ams Nim Paper Draft

AMS-02/TOF

!"#Sg!

!!

Figure 2.106: Charge measurements by the RICH and TOF (2002 test beam).

!

!!

Figure 2.107: Time of Flight Resolution with C2 and C3 vs. particle charge.

81)0!?3'*(!=(!\!u!%FQ!<3>>0;?3*A;!(3!(B3!?0=O!"?!'*!5'7C>0!"F%.Q:F

Page 129: 2004 Ams Nim Paper Draft

AMS-02/TOF

! "#Sc

2.4.6 References

L%M! WF!J366'*'!0(!=6F/!HC3@3!^'20*(3!61A!8%SgS:!%"Ub!

+F!\'<)'<)'/!+**=6;!34!P)D;'<;!66!8%Sc%:!Q.Ub!

+F!\'<)'<)'/!q-(CAD!34!<)=>70A!4'*=6!;(=(0;!?>3AC<0A!'*!0a0#!'*(0>=<('3*;r!'*!qT6020*(=>D!

?>3<0;;0;!=(!_'7)!T*0>7Dr/!+<=A02'<!P>0;;!8%Sc%:/!?F!cS.b!

,F!J=;'60!0(!=6F/!HC<6F!G*;(>C2F!=*A!,0()F!179!8%S$%:!QccF!

L"M! WF!+6@';'!0(!=6F/!HC<6F!G*;(>C2F!=*A!,0()F!+!437 8%SSS:/!"%"F!

LdM! IFJ>3<<3!0(!=6F/!P>3<F!"c()!!G^]^!8"..%:!"%SdF!

LQM! eF!I0@'!0(!=6/!P>3<F!$()!G^+1PP/!^323/!G(=6D/!"..dF!!!

LUM! JF!J0*<)0'O)!0(!=6F/!HC<6F!G*;(>C2F!=*A!,0()F!+!315!8%SS":!dQSF!

LgM! HF^=>3(=/!q-(CA'!?0>!6=!<=6'E>=R'3*0!0!6k3(('2'RR=R'3*0!A0'!43(3236('?6'<=(3>'!?0>!'!<3*(=(3>'!=!

;<'*('66=R'3*0!A0663!;?0((>320(>3!;?=R'=60!+,-#."r/!I=C>0=!1)0;';/!J3637*=!8"..":F!

!

Page 130: 2004 Ams Nim Paper Draft

AMS-02/ACC

2-98

2.5 Anticoincidence Counters (ACC) The AMS-02 Silicon tracker is surrounded by a layer of scintillation counters fitting tightly inside

the inner bore of the superconducting magnet (see Figure 2.1), developed by RWTH-Aachen. Sixteen

scintillation panels (BICRON BC414) of 8 mm thickness form the ACC (Figure 2.108). The panels

dovetail along their vertical joints (Figure 2.108 inserts) to provide hermetic coverage. The ACC detects

particles which enter the tracker laterally, outside of the main acceptance. Those particles may confuse

the charge determination if they leave hits in the tracker close to the tracks of interest. The ACC

scintillation counters are designed such that they can reject unwanted particles with high efficiency.

Furthermore the photomultipliers (PMTs) that record the light signals from the ACC panels have to work

in a moderate (~1.2 kG) magnetic field at locations on the top of and on the bottom of the magnet vacuum

case, approximately 40 cm from the racetrack coils (Figure 2.109). To minimize the impact of this, the

mesh PMTs (Hamamatsu R5946) are oriented with their axes parallel to the stray field. The light from

the scintillation panels is collected in wavelength shifter fibers (Kuraray Y-11(200)M, diameter 1 mm)

embedded in grooves milled into the scintillation panels (Figures 2.108, 2.110 and 2.111). The embedded

fibers are collected into 2 output ports of 37 fibers each at both ends of the counters (Figure 2.111). For

each panel there are two transition connectors (Figure 2.112), located on the upper and lower conical

flanges of the magnet vacuum case. From these transition connectors the light is routed through clear

fibers up to the PMTs mounted on the rim of the vacuum case.

Figure 2.108: Anticounter scintillation panel. The edges are dovetailed for hermeticity.

Page 131: 2004 Ams Nim Paper Draft

AMS-02/ACC

2-99

Figure 2.109: ACC light transport system, from the fibers embedded in the panels, through the

couplings to the PMTs located on the outer rim of the vacuum case.

The light signal provided by the closely spaced wavelength shifter fibers and transported further

on by the clear fibers to the PMTs typically yields 15 to 20 photoelectrons. One track thus results in at

least 30 photoelectrons for detection since there are 2 tubes connected to each counter. For minimum

ionizing particles at normal incidence to the panels, the mean electrical output charge of the PMTs is

13 pC. The front end electronics of the ACC is identical to that of the TOF system (see § 2.4.3). Signals

from the ACC are included in the AMS-02 trigger in order to optimize the trigger performance by

rejecting events outside the tracker acceptance.

A prototype counter has been tested with 10 GeV protons at CERN in 2003. Figure 2.113 shows

a sample of the pulse height distributions observed within 3 cm of the edge. Figure 2.113a shows the

typical upward fluctuations generally observed in energy loss measurements of charged particles. In

order to emphasize the low signal behavior, Figure 2.113b, displays the spectrum below the most

probable energy loss. Two different trigger conditions are displayed: for the events in red one of

adjacent counters was required to have a signal; for the events in yellow only the beam defining counters

were required. In the first case, a signal was observed in the counter under test for each of the 350,000

proton events. In the second case approximately 45 events were below threshold (0.6 pC). With this

performance, the ACC guarantees that an antimatter signal will not be simulated due to laterally entering

particles.

Page 132: 2004 Ams Nim Paper Draft

AMS-02/ACC

2-100

Figure 2.110: ACC during machining of the fiber grooves.

Figure 2.111: Finished ACC panel end.

Page 133: 2004 Ams Nim Paper Draft

AMS-02/ACC

2-101

Figure 2.112: ACC light cable connectors, wave length shifter fibers arrive from the

panel on the right side, clear fibers continue to the PMT on the left.

Figure 2.113: ACC prototype test with 10 GeV protons. a) Pulse height spectrum

from typical run, counts vs. PMT charge. b) Pulse height spectrum

below maximum, counts vs. charge, with tight (red) and loose (yellow)

trigger conditions (see text).

Page 134: 2004 Ams Nim Paper Draft

AMS-02/RICH

!"#$%"!

2.6 Ring Imaging Cerenkov Detector (RICH) &'!()*+)!,(!-,.*/!0.'*12+',13!,(456-!5'!1-,)(41),563+!47/-56-!-.67!1-!,7+!+85-,+'6+!(0!1',521,,+)!()!

,7+! )+31,59+! 1:.'*1'6+-! (0! 35;7,! 5-(,(4+-! 1'*! 671);+*! '.63+5<! 5,! 5-! '+6+--1)/! ,(! 719+! 1! 4)+65-+!

*+,+)25'1,5('!(0!,7+!21--+-!(0!671);+*!41),563+-=! !>7+!21--!(0!1!41),563+!5-!)+31,+*!,(!5,-!2(2+',.2<!p<!

1'*! 9+3(65,/<! *<! ,7)(.;7! ,7+! +84)+--5('! "#$?@A **pm 2 ! 1'*! 5,-! *+,+)25'1,5('! 5-! :1-+*! ('! ,7+!

2+1-.)+2+',! (0! :(,7! B.1',5,5+-=! ! &'! ,7+! CDE! -4+6,)(2+,+)<! ,7+! 2(2+',.2! 5-! *+,+)25'+*! 0)(2! ,7+!

5'0()21,5('! 4)(95*+*! :/! ,7+! E5356('! >)16F+)! G5,7! 1! )+31,59+! 166.)16/! (0! ?$H! (9+)! 1! G5*+! )1';+! (0!+'+);5+-=!!>75-!+',153-!1'!+))()!(0!,7+!-12+!()*+)!('!,7+!21--!(0!,7+!41),563+!-(<!5'!()*+)!,(!(9+)6(2+!,75-!

.'6+),15',/<!,7+!9+3(65,/!71-!,(!:+!2+1-.)+*!G5,7!1!)+31,59+!166.)16/!(0!1:(.,!$!4+)!253=!!I()!,75-!4.)4(-+!

1!J5';! &21;5';!K+)+'F(9!L+,+6,()! AJ&KM?! 71-! :++'! *+-5;'+*!G5,7! 1! 31);+! ;+(2+,)5613! 166+4,1'6+! ,(!

(4+)1,+!5'!,7+!+'95)('2+',13!6('*5,5('-!(0!,7+!(.,+)!-416+=!!!

>7+!*+,+)25'1,5('!(0!,7+!9+3(65,/!(0!671);+*!41),563+-!5-!:1-+*!('!,7+!K+)+'F(9!+00+6,=!!N7+'!1!

671);+*!41),563+!;(+-!,7)(.;7!1!*5+3+6,)56!21,+)513<!5,!5'*.6+-!1!216)(-6(456!4(31)5-1,5('=!!&0!5,-!9+3(65,/!5-!

31);+)!,71'!,7+!471-+!9+3(65,/!(0!,7+!+3+6,)(21;'+,56!05+3*!5'!,7+!21,+)513<!,7+!671';+!(0!,7+!*54(31)!05+3*-!

G5,7!,52+!5'5,51,+-!,7+!+25--5('!(0!+3+6,)(21;'+,56!)1*51,5('=!!>7+!*500+)+',!2('(67)(21,56!G19+-!+25,,+*!

5'!,7+!(4,5613!)+;5('!(0!,7+!21,+)513!0()2!132(-,!,7+!-12+!1';3+!G5,7!)+-4+6,!,(!,7+!9+3(65,/!(0!,7+!41),563+=!!

>7+)+0()+<!1!6('+!(0!K+)+'F(9!)1*51,5('!5-!6)+1,+*!13(';!5,-!,)1O+6,()/!5'!,7+!21,+)513=!!>7+!4)(4+),5+-!(0!

,75-!)1*51,5('!6('+!*+4+'*!('!,7+!9+3(65,/!(0!,7+!671);+*!41),563+!1'*!,7+!)+0)16,59+!5'*+8!(0!,7+!21,+)513<!

n(()=!!&'!41),56.31)<!0()!1'!5'6(25';!41),563+!(0!671);+!P+<!,7+!7130!(4+'5';!1';3+!(0!,7+!6('+!5-!;59+'!:/!

?A@$6(- (*@ n2 Q!,7+!'.2:+)!(0!)1*51,+*!47(,('-!5'!1!0)+B.+'6/!)1';+!d(!0()!1!,)19+)-+*!3+';,7!dx!5'!,7+!

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-4+6,)(2+,+)<! :+,G++'! ,7+! 3(G+)! >52+! (0! I35;7,! K(.',+)-! 1'*! ,7+! R3+6,)(21;'+,56! K13()52+,+)=! ! &,! 5-!

:+5';!:.53,!:/! &SIS#T(3(;'1!.'*+)!6(',)16,! ,(! ,7+! &,1351'!E416+!C;+'6/!ACE&?<!K&RDC><! &'-,5,.,(!*+!

C-,)(05-561!*+!K1'1)51-<!U1:=!&'-,=!R84=!V1),563+!V7/-56-<!W=!(0!D1)/31'*<!I3()5*1!CXD<!S1,=!C.,(=!W=!(0!

D+856(!1'*!UVEK=!!C-!-7(G'!5'!I5;.)+!"=$$Y<!,7+!J&KM!71-!1!,).'61,+*!6('5613!-714+!G5,7!Z%!62!.44+)!

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,756F'+--!31/+)!(0!*5+3+6,)56!21,+)513!A)1*51,()?=!!>7+!3(G+)!431'+<!G7567!71-!1!ZY8ZY!62"!-B.1)+!6+',)13!

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,7+!47(,('!*+,+6,()-!5'!,7+!3(G+)!431'+=!!>7+!(,7+)!47(,('-!1)+!)+03+6,+*!('!,7+!31,+)13!-.)016+!(0!,7+!6('+!

1'*!13-(!*5)+6,+*!,(!,7+!47(,('!*+,+6,()-=!!C,!,7+!3(G+)<!()!521;+<!431'+<!,7+!47(,('!*+,+6,()-!719+!35;7,!

;.5*+-! 1,,167+*! ,(! 47(,(#2.3,5435+)! ,.:+-! AVD>-?=! ! I)(2! ,7+! -41,513! 6(()*5'1,+-! (0! ,7+! 47(,(2.3,5435+)!

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,7+!41),563+!*+,+)25'+*=!!W4G1)*!;(5';!41),563+-!*(!'(,!3+19+!,75-!-5;'13!1'*!61'!,7.-!:+!.'12:5;.(.-3/!

*5-6)525'1,+*=!!!!

Page 135: 2004 Ams Nim Paper Draft

AMS-02/RICH

! "#$%\

!!

Figure 2.114: The main structural components of the RICH.

2.6.1 Radiator

E+9+)13!*5+3+6,)56!21,+)513-!719+!:++'!6('-5*+)+*!1-!4(--5:3+! )1*51,()-=! !>7+5)!4+)0()21'6+!71-!

:++'!1'13/-+*!:/!1!D(',+!K1)3(!-52.31,5('!1'*<!0()!,7+!2(-,!144)(4)51,+!('+-<!,+-,-!719+!:++'!4+)0()2+*!

G5,7! 5('! :+12-! 1,! KRJS! 1'*! 6(-256! )1/-! 1,! UVEK! A^)+'(:3+?=! ! >7+! 21,+)513! ,71,! 71-! -7(G'! :+,,+)!

4+)0()21'6+!0()!,7+!+84+)52+',13!;(13-!1)+!-53561!C+)(;+3-=!!>7+-+!6(24(.'*-!1)+!1!258,.)+!(0!mAE5_"?!

1'*!"mAM"_?<!G5,7!m!1'! 5',+;+)<!1'*!719+!1!4()(.-!-,).6,.)+!G5,7!:.::3+-<!2(-,!(0! ,7+2!(0!-2133!-5`+!

6(241)+*! ,(! (4,5613!G19+3+';,7-=! ! >7+! )+0)16,59+! 5'*+8! 5-! 1'! 19+)1;+! :+,G++'! ,7+! ('+-! (0! 15)! 1'*! ,7+!

258,.)+! 1'*! 71-! 1'! 132(-,! 35'+1)! *+4+'*+'6+!G5,7! ,7+! *+'-5,/=! !>7.-<!G5,7! *500+)+',! ,)+1,2+',-! (0! ,7+!

258,.)+! 144)(4)51,+!*+'-5,5+-! 61'!:+! -+3+6,+*! 5'! ,7+! )1';+!(0!%=$! ,(!%=\!;! 62!\! 1'*! ,7+)+0()+! )+0)16,59+!

5'*56+-!;)+1,+)!,71'!2(-,!;1-+-!1'*!-2133+)!,71'!2(-,!35B.5*-!1'*!-(35*-!61'!:+!(:,15'+*=!!>7+)+!1)+!,G(!

-.4435+)-!(0!75;7!B.135,/!C+)(;+3-!G5,7! ,7+!*+-5)+*!4)(4+),5+-! A-++!>1:3+!"=Y?a! ,7+!K1,13/-5-! &'-,5,.,+!(0!

S(9(-5:5)-F! A7+)+10,+)! )+0+))+*! 1-! K&S?<! G7567! 4)(*.6+-! \!62! ,756F! 7/*)(475356! ,53+-<! 1'*!D1,-.-75,1!

R3+6,)('56!K(241'/!!ADRK?!G7567!4)(*.6+-!7/*)(47(:56!,53+-!(0!$!62!,756F'+--=!!!

!

Supplier Refractive IndicesClarity

(mm4/cm)

Size

(cm3)

Other

features

DRK! $=%\!b!$=%c! %=%%[!b!%=%$\! $$=c!8!$$=c!8!$! M/*)(47(:56!

K&S! $=%\!b!$=%c! %=%%c!b!%=%%]! $$=c!8!$$=c!8!\! M/*)(475356!

!

Table 2.4: Properties and manufacturers of high quality silica Aerogel.

!

Page 136: 2004 Ams Nim Paper Draft

AMS-02/RICH

!"#$%Y!

E+9+)13! ,53+-! 4)(*.6+*! :/! ,7+! ,G(! 21'.016,.)+)-! 719+! :++'! ,+-,+*! .'*+)! *500+)+',! +8,+)'13!

6('*5,5('-=!!&'!41),56.31)<!2+671'5613!1'*!(4,5613!4)(4+),5+-!-.67!1-!,7+!)+0)16,59+!5'*+8<!,7+!,)1'-25,,1'6+!

1'*! ,7+! 35;7,! *5-4+)-5('!G+)+! 1'13/-+*!:/! +84(-5';! ,7+! ,53+-! ,(! ,7+)213! 1'*!916..2!6/63+-! 5'! ()*+)! ,(!

1--+--! ,7+! 4+)0()21'6+! (0! ,7+! )1*51,()! .'*+)! ,7+! +8,)+2+! +'95)('2+',13! 6('*5,5('-! (0! (.,+)! -416+=! ! &'!

()*+)!,(!5'6)+1-+!,7+!47(,('!*+,+6,5('!+00565+'6/!0()!,7(-+!41),563+-!,71,!0133!.4('!,7+!6+',)13!7(3+!(0!,7+!

*+,+6,5('! 431'+<! ,7+! 6+',)13! :3(6F-! (0! ,7+! )1*51,()! 1)+!21*+! (.,! (0!S1I<!G7567! 71-! 1! 75;7+)! )+0)16,59+!

5'*+8! And$=\\Z?! 1'*! -(! ;59+-! 1!G5*+)! K+)+'F(9! 6('+=! ! >7.-<! ,7+!2+671'5613! -,).6,.)+! (0! ,7+! )1*51,()!

6('-5-,-!(0!]%!)+6,1';.31)!:3(6F-!(0!-53561!C+)(;+3!(0!$$=c8$$=c8\!62\!1'*!$Z!6+',)13!:3(6F-!(0!S1I!(0!

]=c8]=c8%=c!62\=! !C33! ,7+!:3(6F-!1)+!-.44(),+*!0)(2!,7+!:(,,(2!:/!1!$!22!,756F! 31/+)!(0!2+,716)/31,+!

0)++!(0!We!1:-():5';!1**5,59+-!,71,!5-!058+*!,(!,7+!>_I!.44+)!-.44(),5';!431'+=!!!

!

2.6.2 Reflector

C:(.,!\%H!(0!,7+!K+)+'F(9!47(,('-!+2+);5';!0)(2!,7+!)1*51,()!1)+!4(5',+*!(.,-5*+!(0!,7+!47(,('!

*+,+6,()!1))1/=!!C!)+03+6,()!A-++!I5;.)+!"=$$c?!71-!:++'!*+-5;'+*!,(!6(33+6,!,7(-+!47(,('-!5'!,7+!1))1/=!!&,!

6('-5-,-! (0! 1! -.44(),5';! -,).6,.)+!G5,7! 1! ,).'61,+*! 6('5613! -714+! (0! $\Y! 1'*! $$Y! 62! 3(G+)! 1'*! .44+)!

*512+,+)-!1'*!1! ,75'!0532!(0! )+03+6,59+!6(1,5';!*+4(-5,+*!('! ,7+! 5''+)!-.)016+=! ! &'!()*+)! ,(!215',15'! ,7+!

$ 4+)!253!9+3(65,/!)+-(3.,5('<!5,!71-!:++'!*+-5;'+*!G5,7!-,)(';!)+B.5)+2+',-!('!,7+!,(3+)1'6+-!1-!-7(G'!5'!

>1:3+!"=c=!!!

!

K('565,/! "%%!-2K+',+)5';! $%%!-2J+03+6,595,/! B ]c!H!A1,!C d!Y"%!'2?J(.;7'+--! D $c%!'2E3(4+!+))()! f!$!2)1*!

!

Table 2.5: Parameters and designed tolerances for the reflector.

C-!-7(G'!5'!I5;.)+!"=$$c<!,7+!)+03+6,()!5-!4)(*.6+*!5'!$"%#*+;)++!6(24(-5,+!-+;2+',-<!G7567!1)+!

0)12+*!G5,7!6(24(-5,+! )5:-!1,! ,7+!+',5)+!4+)52+,+)!(0! ,7+!25))()=! !>7+!6(24(-5,+!.-+*! 5-!TJg>R!!Rh#

$c$c@Dcci! U125'1,+! G5,7! W'5*5)+6,5('13! V)+4)+;! ;3.+*! G5,7! DCE>RJ! T_SL! RV\%U>R#U_! R4(8/!

C*7+-59+=!!>7+!:.-75';!5-!-,15'3+--!-,++3=!!&'!()*+)!,(!1675+9+!,7+!)+03+6,595,/!)+B.5)+2+',<!,7+!)+03+6,59+!

6(1,5';!5-!21*+!.4!(0!$%%!'2!(0!13.25'5.2!1'*!\%%!'2!(0!E5_"=!!!

!!

Figure 2.115: The conical reflector of the Cerenkov detector (3 sectors layout).

!

>7+!)+03+6,()!5-!21*+!:/!1!)+43561!,+67'5B.+=!!>7+!-,1),5';!4(5',!5-!1!21'*)+3!A1!*5+?!('!G7567!,7+!

KIJK!435+-<!G7567!G533! :+! ,7+! 31,+)13! -.)016+!(0! ,7+! )+03+6,()<! 1)+! 4(-5,5('+*!:+0()+!:+5';! 6.)+*=! !>7+!

21'*)+3!1'*!435+-!1)+!(9+'!6.)+*!.'*+)!916..2!1'*!,7+'!,7+!-.)0165';!4)(6+--!:+;5'-=!!W-5';!1!41,+',+*!

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AMS-02/RICH

! "#$%c

,+67'5B.+<! 1! ,75'! 31/+)! A1! 0+G! ,+',7-! (0! 1! 253352+,+)?! (0! )+-5'! 5-! 4(.)+*! :+,G++'! ,7+! KIJK! 1'*! ,7+!

21'*)+3=!!C0,+)!1!-+6('*!6.)+!4)(6+--<!,7+!2+671'5613!41),!(0!,7+!31,+)13!-.)016+!5-!)+1*/=!!&,!5-!524(),1',!

,(! 719+! 1! 21'*)+3! G5,7! ,7+! +816,! -714+<! *52+'-5('-! 1'*! )(.;7'+--! (0! ,7+! )+03+6,()! ,(! :+! 4)(*.6+*=!!

C0,+)G1)*-! ,7+! 031';+-! 1'*! ,7+! )5:-! 1)+!;3.+*! ,(! ,7+! 31,+)13! -.)016+!.-5';! ,7+!21'*)+3! 1-! 1!;+(2+,)5613!

)+0+)+'6+=! ! I(33(G5';! ,75-! 4)(6+*.)+<! ,7+! ,7)++! -+6,()-! 1)+! 4)(*.6+*! 1'*! ,7+'! 1--+2:3+*! :/!;3.5';! ,7+!

9+),5613!)5:-!.-5';!,7+!21'*)+3!1-!1!O5;=!!>7+!05'13!-,+4!5-!,7+!6(1,5';!21*+!:/!916..2!*+4(-5,5('!(0!,7+!

13.25'.2!1'*!-5356('!*5(85*+!31/+)-=!!!

>7+!21'*)+3!0()!,7+!05'13!25))()!71-!:++'!4)(*.6+*!AI5;.)+!"=$$Z?=!!_4,5613!2+1-.)+2+',-!719+!

-7(G'!,71,!,7+!-.)016+!)(.;7'+--!5-!3+--!,71'!$c!'2!1'*!,71,!133!,7+!)+B.5)+*!,(3+)1'6+-!1)+!-1,5-05+*=!!&,!

71-!:++'!.-+*!,(!4)(*.6+!,G(!-1243+-!(0!,7+!)+03+6,()!A(0!\%!8!Yc!62?!,(!,+-,!,7+!(4,5613!4)(4+),5+-<!('+!(0!

G7567!G1-!.-+*!5'!,7+!4)(,(,/4+!,+-,-=!!>7+!2+1-.)+*!)(.;7'+--!(0!,7+!-.)016+!G1-!3+--!,71'!c=\!'2!A)2-?!

1'*!,7+!)+03+6,595,/!;)+1,+)!,71'!]cH!1,!Y"%!'2=!!C0,+)!,7+-+!)+-.3,-<!('+!(0!,7+!,7)++!-+;2+',-!(0!,7+!05'13!

25))()!71-!:++'!4)(*.6+*!:/!K(24(-5,+!D5))()!C443561,5('-!&'6=!A>.6-('<!CP?!G5,7!1!)(.;7'+--!(0!3+--!

,71'!\=]!'2=!!!

!

!!

Figure 2.116: Measurement of the mandrel and a sample produced

to control the roughness and reflectivity.

!

2.6.3 Photon detection system!

>7+! K+)+'F(9! 47(,('-! 1)+! 6(33+6,+*! 1,! ,7+! :(,,(2! (0! ,7+! *+,+6,()! :/! 1'! 1))1/! (0! Z]%!

47(,(2.3,5435+)!,.:+-!AVD>-?!,71,!G5,7-,1'*!2(*+)1,+!21;'+,56!05+3*-=!!M(G+9+)<!,7+!)+-5*.13!05+3*!(0!,7+!

-.4+)6('*.6,5';!21;'+,!5'!,7+!)+;5('!G7+)+!,7+!47(,(2.3,5435+)-!1)+!4316+*!5-!E!\%%!^!-(!,7+/!719+!,(!:+!-.))(.'*+*! :/! 1! -75+3*5';! 61-+! 1'*<! 1-! 1! 6('-+B.+'6+<! 1! 35;7,! 6(33+6,5('! -/-,+2!71-! ,(! :+! *+-5;'+*! 5'!

()*+)! ,(! *5)+6,! ,7+! K+)+'F(9! 47(,('-! 0)(2! ,7+! ,(4! (0! ,7+! -75+3*5';! 61-+! ,(! ,7+! -+'-5,59+! 41),! (0! ,7+!

47(,(2.3,5435+)-=!!>7.-!+167!.'5,!(0!,7+!47(,('!*+,+6,5('!-/-,+2<!1-!-7(G'!5'!I5;.)+!"=$$[<!5-!6(24(-+*!

(0!1!47(,(2.3,5435+)<!,7+!-75+3*5';<!,7+!7(.-5';!1'*!,7+!35;7,#;.5*+-=!!!

>(! *+,+6,! ,7+! K+)+'F(9! 47(,('-<! *500+)+',! 47(,(2.3,5435+)! ,.:+-! 719+! :++'! 1'13/-+*=! ! D(-,!

144)(4)51,+! 0()! ,7+! 671)16,+)5-,56-! (0! ,75-! *+,+6,()! 5-! ,7+! MCDCDC>EW! J[Z%%#%%#D$Z! *.+! ,(! ,7+!

)+*.6+*! -5`+<! 01-,! )+-4('-+! .'*+)! 3(G! (4+)1,5('13! 9(3,1;+! A]%%!e?<! 31);+! 1'(*+! .'50()25,/! 1'*! 3(G!

-+'-5,595,/!,(!+8,+)'13!21;'+,56!05+3*-=!!>7+!K+)+'F(9!47(,('-!1)+!*+,+6,+*!('!,7+!521;+!431'+!1,!Y%!62!

0)(2! ,7+! )1*51,()! 21,+)513=! >7+)+0()+! ,7+! 166.)16/! 5'! ,7+! 2+1-.)+2+',! (0! ,7+! 9+3(65,/! *+4+'*-!

-5;'50561',3/!('!,7+!-5`+!(0!,7+!47(,('!-+'-()-=!!>7+!10()+2+',5('+*!47(,(2.3,5435+)-!719+!1!2.3,51'(*56!

-,).6,.)+!G5,7!Y!8!Y!458+3-<!+167!('+!G5,7!1!-+'-5,59+!`('+!(0!Y!8!Y!22"=!!>75-!;.1)1',++-!1!)+-(3.,5('!5'!

,7+!2+1-.)+2+',!(0!,7+!9+3(65,/!(0!$!4+)!253=!!>7+-+!VD>-!13-(!719+!1!75;7!B.1',.2!+00565+'6/!AE"%H?!

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AMS-02/RICH

!"#$%Z!

5'! 1! )1';+!(0!G19+3+';,7-!:+,G++'!\%%!1'*!Z%%!'2<!G+33!G5,75'! ,7+!(4,5613! )+;5('!(0! ,7+! )1*51,()! 1'*!

G7+)+!,7+!)+0)16,59+!5'*+8!5-<!,(!1!31);+!+8,+',<!5'*+4+'*+',!(0!,7+!47(,('!+'+);/=!!N5,7!,75-!+00565+'6/<!

0()!1'!.3,)1!)+31,595-,56!41),563+!(0!671);+!P!d!$<!1'!19+)1;+!(0!]!47(,('-!1)+!*+,+6,+*!0()!1!)1*51,()!G5,7!1!

)+0)16,59+! 5'*+8! (0! nd$=%\=! !N+! 719+! 1'13/-+*! +167! 47(,(2.3,5435+)! 0()! ,7+! *+,+6,()! .'*+)! -5';3+! 1'*!

2.3,543+!47(,('!+865,1,5('-!1'*!671)16,+)5-+*!,7+5)!)+-4('-+!5'!,+)2-!(0!,7+!;15'<!,7+!-4)+1*!(0!6(33+6,+*!

671);+!1'*!,7+!35'+1)5,/!5'!()*+)!,(!+B.135`+!,7+5)!)+-4('-+!G5,75'!,7+!75;7!9(3,1;+!)1';+!(0![c%!,(!]c%!e=!

!

!!

Figure 2.117: The photon detection system and an exploded view of the main components.

!

>(!+'-.)+! ,7+!VD>!4+)0()21'6+<!+167!('+!5-!4316+*<! ,(;+,7+)!G5,7! ,7+!6())+-4('*5';!0)(',#+'*!

+3+6,)('56!:(1)*-<!5'-5*+!1!6+33!21*+!(0!-(0,!5)('!1'*!eCK_IUWh!c%<!1!*5121;'+,56!21,+)513!,71,<!10,+)!

4)(4+)! 1''+135';<! 4)(95*+-! ;((*! -75+3*5';! 5'! -,)(';!21;'+,56! 05+3*-=! ! >7+! *52+'-5('-! (0! ,7+! 6+33-! 1)+!

3(';+)! ,71'!,7(-+!(0! ,7+!47(,(2.3,5435+)! ,(!19(5*!:(.'*1)/!+00+6,-=!L.+!,(! ,7+!;+(2+,)/!(0! ,7+!1))1/!(0!

47(,(2.3,5435+)-<!,7+/!1)+!1--+2:3+*!0()25';!1!;)5*!G5,7!,G(!*500+)+',!;+(2+,)5+-a!-B.1)+!AG5,7!$Y\!6+33-?!

1'*! ,)51';.31)! AG5,7!"[!6+33-?=! !>7+!*500+)+',!;)5*-!1)+! -.44(),+*!:/!1! -+6('*1)/! -,).6,.)+!21*+!(.,!(0!

13.25'5.2!:+12-!,71,!13-(!7(3*!,7+!0).-,.2!(0!,7+!6('5613!)+03+6,()=!!N+!719+!1'13/-+*!,7+!4+)0()21'6+!

(0! ,7+! -75+3*5';! 61;+! .'*+)! 1'! +8,+)'13! 21;'+,56! 05+3*! (0! \%%!^! A,7+! 21852.2! .'*+)! G7567! ,7+!

47(,(2.3,5435+)-!G533!719+! ,(!(4+)1,+?!1'*!*500+)+',!()5+',1,5('-=! ! &'! ,7+!G()-,!61-+<! ,7+! 5''+)! 05+3*!G1-!

13G1/-!3+--!,71'!$"%!^=! !R167!VD>!G1-!,+-,+*!5'*+4+'*+',3/!,(!+-,1:35-7!5,-!4)(4+)!4+)0()21'6+!.'*+)!

,75-!)+-5*.13!05+3*=!!C-!,7+!+3+2+',-!(0!,7+!;)5*!1)+!058+*!,(;+,7+)!:/!-4(,!G+3*5';<!1!-+)5+-!(0!2+671'5613!

2+1-.)+2+',-! 719+! :++'! 4+)0()2+*! ,(! +'-.)+! ,71,! ,7+! ,7+)213! -,)+--! -(! 5'*.6+*! *(+-! '(,! -5;'50561',3/!

2(*50/!,7+!*5121;'+,56!4)(4+),5+-!(0!,7+!21,+)513-=!

>7+!5',+)016+!:+,G++'!,7+!47(,(2.3,5435+)-!1'*!,7+!G133-!(0!,7+!-75+3*5';!;)5*!5-!1!4(3/61):('1,+!

:(8! A7(.-5';?! ,71,! 13-(! 6(',15'-! ,7+! 0)(',#+'*! +3+6,)('56-! :(1)*-=! ! >7+! 7(.-5';! 71-! :++'! *+-5;'+*! ,(!

+'-.)+! ,7+!135;'2+',!(0! ,7+!47(,(2.3,5435+)!458+3-!1'*!,7+! 35;7,!;.5*+-!G5,75'!,7+!-75+3*5';!6+33-=! !T(,7!

1)+!;3.+*!,(!,7+!7(.-5';!1'*<!5'!133!4(--5:3+!6('05;.)1,5('-<!1!6())+6,!135;'2+',!71-!:++'!1675+9+*=!!!

>7+!35;7,!6(33+6,5('!-/-,+2!3+1*-!,7+!K+)+'F(9!47(,('-!0)(2!,7+!,(4!(0!,7+!-75+3*5';!61-+!,(!,7+!

-+'-5,59+!41),!(0! ,7+!47(,(2.3,5435+)-=! !L500+)+',!(4,5('-!719+!:++'!1'13/-+*a! 05:+)!(4,56!61:3+-<!7(33(G!

35;7,!;.5*+-!G5,7!)+03+6,5';!5''+)!-.)016+-!1'*!-(35*!35;7,!;.5*+-!G()F5';!:/!5',+)'13!)+03+6,5('=!!L+,153+*!

D(',+!K1)3(! -52.31,5('-! 719+! -7(G'! ,71,<! 0()! ,7+! 16,.13! *52+'-5('-! (0! ,7+!K+)+'F(9!*+,+6,()! 1'*! ,7+!

41),56.31)!671)16,+)5-,56-!(0!,7+!)1*51,()<!,7+!-(35*!35;7,!;.5*+-!1)+!,7+!2(-,!+00565+',=!!M(G+9+)<!,7+!(4,5613!

1'*! 2+671'5613! 4)(4+),5+-! (0! ,7+! 431-,56! 1)+! 6).6513! 0()! ,7+! ;((*! 4+)0()21'6+! (0! ,7+! 35;7,! 6(33+6,5('!

!

Shielding Electronics

Light guide

PMT

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AMS-02/RICH

! "#$%[

-/-,+2=! ! >7+! 47(,(2.3,5435+)! )+-4('-+! 71-! 75;7! B.1',.2! +00565+'6/! 0()!G19+3+';,7-! :+,G++'! \%%! 1'*!

Z%%!'2=! !_'! ,7+!(,7+)!71'*<!*.+! ,(! ,7+!1';.31)!*5-,)5:.,5('!(0! ,7+! 5'6(25';!47(,('-<! ,7+!19+)1;+!41,7!

3+';,7!5'-5*+!,7+! 35;7,!;.5*+-! 5-!\=[!62=! !>7+)+0()+<!G+!)+B.5)+!1! ,)1'-25,,1'6+!1-!75;7!1-!4(--5:3+!(9+)!

,75-! G19+3+';,7! 5',+)913Q! 5'! 41),56.31)<! 21,+)513-! 0)++! 0)(2! We! 1:-():5';! 1**5,59+-! 2.-,! :+! .-+*=!!

I.),7+)2()+<!,7+!)+0)16,59+!5'*+8!71-!,(!:+!1-!63(-+!1-!4(--5:3+!,(!,7+!('+!(0!,7+!47(,(2.3,5435+)!G5'*(G!

An d!$=c?<! ,7+! *+'-5,/! 3(G! ,(! 25'525-+! ,7+! G+5;7,! (0! ,7+! G7(3+! -,).6,.)+! 1'*! ,7+! ,7+)213! +841'-5('!

6(+00565+',! -2133! ,(! G5,7-,1'*! ,+24+)1,.)+! ;)1*5+',-! G5,7(.,! -5;'50561',! *+0()21,5('=! ! D1'/! *500+)+',!

();1'56!21,+)513-!719+!:++'!1'13/-+*!1'*!L&Cj_S!U^#[%\!G1-!-+3+6,+*=!!&'!()*+)!,(!)+*.6+!,7+!3(--+-!

61.-+*!:/! ,7+!*500+)+',!(4,5613! 5',+)016+-<! 1! ,75'! 0532! A$!22?!(4,5613! O(5',! 5-! 5'-+),+*!:+,G++'! ,7+! 35;7,!

;.5*+-!1'*!,7+!47(,(2.3,5435+)!G5'*(G=!!C-!-7(G'!5'!I5;.)+!"=$$]<!+167!47(,(2.3,5435+)!71-!Y!8!Y!458+3-!

1'*!+9+)/!35;7,#;.5*+!-,).6,.)+!71-!$Z!5'*+4+'*+',!.'5,-!G5,7!Y!*500+)+',!-714+-!1'*!0533-!1!,(,13!9(3.2+!(0!

$\!62\=!!>7+!(4,52.2!*52+'-5('-!719+!:++'!*+,+)25'+*!,(!218525-+!,7+!47(,('!6(33+6,5('!+00565+'6/=!!C!

D(',+!K1)3(!-52.31,5('!(0!*500+)+',!47/-5613!4)(6+--+-!71-!-7(G'!,71,!-.00565+',!K+)+'F(9!47(,('-!1)+!

6(33+6,+*!,(!1675+9+!1!)+-(3.,5('!5'!,7+!9+3(65,/!(0!671);+*!41),563+-!(0!>*!@*!E!$%!b\=!!

!!

Figure 2.118: PMT showing the 4 x 4 anode structure and a 4 x 4 array of light-guides.

K(243+,+! 6+33-<! 1-! -7(G'! 5'! I5;.)+!"=$$[<! G+)+! ,+-,+*! ('! 1! 95:)1,5('! ,1:3+<! I5;.)+!"=$$k<! ,(!

+'-.)+!,71,!,7+!-,).6,.)+!G533!G5,7-,1'*!,7+!-7.,,3+!,1F+#(00=!!>7+!,+-,+*!-,).6,.)+-!:)(F+!:+,G++'!$k!1'*!

"[!;)2-<!\!,(!Y!,52+-!1:(9+!,7+!)+B.5)+*!B.1350561,5('!3+9+3-=!!C!-52531)!,+-,!G1-!4+)0()2+*!('!1'!1--+2:3/!

(0!]!6+33-!1'*!'(!2+671'5613!*121;+!G1-!(:-+)9+*=!!!

!

!

Figure 2.119: Vibration tests of a single cell (left) and of an eight cell array (right).

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AMS-02/RICH

!"#$%]!

2.6.4 Electronics

>7+!+3+6,)('56-!0()!,7+!J&KM!71-!0(.)!215'!6(24('+',-a!0)(',#+'*!+3+6,)('56-<!6(',)(3!1'*!-5;'13!

4)(6+--5';<!2('5,()5';!1'*!-+,,5';!(0!G()F5';!41)12+,+)-!1'*!4(G+)!-.4435+-=!!>7+!0)(',#+'*!+3+6,)('56-!

6('-5-,-! (0! 4)5',+*! 65)6.5,! :(1)*-! 3(61,+*! 1,! ,7+! :1-+! (0! +167! 47(,(2.3,5435+)! A-++! I5;.)+-!"=$$[!

1'*!"=$"%?=!!>7+-+!4)(95*+!,7+!Me!:51-!'+,G()F!0()!,7+!VD>!1'*!,7+!6('*5,5('5';!1'*!*5;5,135`1,5('!(0!

,7+!VD>!1'(*+!-5;'13-=!!>7+!6(',)(3!1'*!-5;'13!4)(6+--5';!-,1;+!5-!*+9(,+*!,(!,7+!;+'+)1,5('!(0!-+B.+'6+-!

(0! 6(',)(3! -5;'13-! ,(! *)59+! ,7+! 0)(',#+'*! +3+6,)('56-! 1'*! ,(! ,7+! 6(331,5('<! )+*.6,5('! 1'*! *5-41,67! (0!

*5;5,5`+*!)+-.3,-=!!&,!6('-5-,-!(0!1!-+,!(0!$"!+3+6,)('56!:(1)*-!3(61,+*!('!,7+!+*;+!(0!,7+!*+,+6,()!-,).6,.)+<!

-7(G'! 5'! ;)++'! 5'! I5;.)+!"=$$Y=! >7+-+! 65)6.5,-! 1)+! :1-+*! ('! ,7+! 6(22('! *5;5,13! 41),! AKLV?! 6.-,(2!

*+9+3(4+*! 0()! CDE! A-++! l!"=]?=! ! >7+! ,75)*! 6(24('+',! *+13-! G5,7! ,7+! 2('5,()5';! 1'*! ,7+! -+,,5';! (0!

*500+)+',! 41)12+,+)-! A35F+! ,+24+)1,.)+<! 9(3,1;+! 1'*! 6.))+',?! :/! 2+1'-! (0! ,G(! +3+6,)('56-! :(1)*-! 13-(!

2(.',+*!('! ,7+!*+,+6,()!+*;+=! !>7+!75;7!9(3,1;+-!)+B.5)+*!:/! ,7+!47(,(2.3,5435+)-!1)+!-.4435+*!:/!('+!

,/4+!(0!.'5,<!2(.',+*!('!,7+!(:35B.+!3+;-!(0!,7+!WEE<!1'*!1!-+6('*!,/4+<!2(.',+*!('!,7+!215'!)1*51,()-<!

4)(95*+-!,7+!*500+)+',!3(G!9(3,1;+-!'++*+*!0()!,7+!)+-,!(0!,7+!+3+6,)('56-=!!

!

!!

Figure 2.120: RICH front end electronics at the base of the PMT.

!

!

i) Front End Electronics

C-!-7(G'!5'!I5;.)+!"=$"%<!,7)++!4)5',+*!65)6.5,!:(1)*-!2(.',+*!('!,7+!:1-+!(0!+167!VD>!0()2!1'!

]%!D#!Me! )+-5-,()! *595*+)!G7567! 4)(95*+-! ,7+! :51-! 0()! +167! */'(*+! (0! ,7+! 47(,(,.:+<! (4,525`5';! ,7+!

4(G+)! 6('-.24,5('! 1'*! 215',15'5';! 1! 9+)/! 75;7! 35'+1)5,/=! ! C'! 1443561,5('! -4+65056! 5',+;)1,+*! 65)6.5,!

ACE&K?! 5-! 2(.',+*! ('! 1! 0(),7! :(1)*! 6(''+6,+*! :/! 1! 03+85:3+! j14,('! 61:3+=! ! >7+! CE&K<! *+9+3(4+*!

-4+65056133/!0()!,7+!CDE#%"!J&KM<!6(',15'-!$Z!671''+3-!(0!1!671);+!-+'-5,59+!4)+1243505+)!G7567!0++*-!

1'!JK#KJ!-714+)!1'*!1!-1243+!X!7(3*!AE@M?!65)6.5,<!G7567!058+-!,7+!21852.2!(0!,7+!-714+*!-5;'13=!!&'!

()*+)!,(!5'6)+1-+!,7+!)+-(3.,5('!0()!,7+!-2133!-5;'13-<!1'!1243505+)<!G7567!-+3+6,-!:+,G++'!1!;15'!016,()!$!

()! c<! 71-! :++'! 1**+*! ,(! ,7+! 6715'=! !C!2.3,543+8+*!(.,4.,! :.00+)! *)59+-! ,7+! -5;'13! ,7)(.;7! 1! 6.))+',! ,(!

9(3,1;+! 6('9+),+)! -71)+*!:/! ,7+! $Z! 671''+3-! (.,!(0! ,7+!CE&K! ,(! 1'! 1'13(;! ,(! *5;5,13! 6('9+),+)! ACLK?=!!

>75-! CLK! AC'13(;! L+956+-! CL]%c$C?<! G7567! 5-! 13-(! .-+*! 5'! ,7+! >JL! 1'*! RKCU! +3+6,)('56-<!

5243+2+',-!1!$"#:5,!-.66+--59+!144)(8521,5('!1,!$!25335('!(0!-1243+-!4+)!-+6('*<!G5,7!3(G!9(3,1;+!1'*!

9+)/!3(G!4(G+)!6('-.24,5('!1'*!-+)513!(.,4.,=!!!

!

!

!

ASIC

HV Divider

Page 141: 2004 Ams Nim Paper Draft

AMS-02/RICH

! "#$%k

ii) Control and Signal Processing Stage

>7+!215'!,)5;;+)!)+;.31,+-!,7+!-1243+!X!7(3*<!,7+!2.3,543+85';!1'*!,7+!CLK!(4+)1,5('-=!!N7+'!

,7+!,)5;;+)!-5;'13!1))59+-<!1! ,)15'!(0!4.3-+-! 5-!4)(*.6+*=!>7+!3+1*5';!4.3-+!4.,-! ,7+!E@M!(0! ,7+!0)(',!+'*!

-,1;+!5',(!-1243+!2(*+!G15,5';!0()!,7+!4+1F!(0!,7+!-5;'13=!!>7+!'+8,!4.3-+!4.,-!,7+!E@M!5',(!7(3*!2(*+!

G15,5';!0()!,7+!-5;'13!,(!:+!)+1*!(.,=!!C,!,7+!3+1*5';!+*;+!(0!+167!-.66+--59+!4.3-+!,7+!(.,4.,!(0!+167!E@M!

5-! ,7+'! -+B.+',5133/! )+1*(.,=! ! &'! 3(6F! -,+4<! ,7+! 1'13(;! ,(! *5;5,13! 6('9+)-5('! 5-! 4+)0()2+*! .-5';! ,G(!

*+*561,+*!63(6F!-5;'13-=! !>7+!05)-,!7(3*-! ,7+!-5;'13!1,! ,7+!CLK!5'4.,!G753+! ,7+!6('9+)-5('!5-!4+)0()2+*!

1'*!,7+!(,7+)!5'5,51,+-!,7+!6('9+)-5('=!!>7+!*5;5,135`+*!-5;'13!5-!,7+'!-+',!,(!1!:.00+)=!!_'6+!,7+!6('9+)-5('!

4)(6+--!5-!6(243+,+*<!,7+!$Z!E@M!5'!,7+!CE&K!1)+!)+-+,!1'*!,7+!CLK!+',+)-!1!3(G!4(G+)!2(*+!.',53!,7+!

'+8,!,)5;;+)=!!>7+!;+'+)1,5('!(0!,7+!6(',)(3!-5;'13-!1'*!,7+5)!-+B.+'6+-!71-!:++'!5243+2+',+*<!1-!-7(G'!

5'!I5;.)+!"=$"$<!,7)(.;7!1'!13;()5,72!71)*G5)+*!5',(!1!)1*51,5('!,(3+)1',<!3(G!4(G+)!1'*!3(G!9(3,1;+!;1,+!

1))1/!ACK>RU!CcYEh["C?=!!!

!

!!

Figure 2.121: RICH Control and signal processing electronics based on CDP design.

C-/'67)('(.-3/! G5,7! ,7+! ,)5;;+)<! ,7+! *1,1! 5-! +8,)16,+*! 0)(2! ,7+! EJCD! :.00+)! 5',(! ,7+! *5;5,13!

-5;'13!4)(6+--()!ALEV?<!4+*+-,13-!1)+!-.:,)16,+*!1'*!,7+!)+-.3,!6(241)+*!,(!1!,7)+-7(3*=!!>7+!4+*+-,13-!1)+!

)+31,+*! ,(! ,7+! +3+6,)('56! (00-+,-! ('! +167! 671''+3! 1'*! ,7+! ,7)+-7(3*! 5-! )+31,+*! ,(! +3+6,)('56! '(5-+=!!

E5;'50561',! *1,1! )+*.6,5('! 5-! 1675+9+*! :/! )+O+6,5';<! ('! 1! ,)5;;+)! :/! ,)5;;+)! :1-5-<! ,7(-+! 671''+3-! G5,7!

12435,.*+-! :+3(G! ,7)+-7(3*=! ! >7+! -+3+6,+*! LEV! AC'13(;! L+956+-! CLEV"$][U#TjE>?! (4+)1,+-! 1,! c%!

D&VE!1'*!5'63.*+-!\"j!G()*-!(0!2+2()/!0()!('!6754!:.00+)5';=!!_'6+!4)(6+--+*<!,7+!*1,1!1)+!-+',!,(!1'!

(.,4.,!:.00+)!.',53!,7+/!1)+!)+1*!(.,!:/!,7+!'+8,!3+9+3!(0!,7+!*1,1!16B.5-5,5('!-/-,+2=!!!

>75-!'+8,!3+9+3!5-!35F+!,7+!65)6.5,!-7(G'!5'!I5;.)+!"=$"$!+86+4,!,71,!,7+!6(''+6,5('-!,(!,7+!VD>-!

1)+!)+4316+*!:/!$%%!DM`!-+)513!4(5',!,(!4(5',!35'F-!,(!+167!(0!,7+!*1,1!)+*.6,5('!65)6.5,-=!!C0,+)!6(331,5('!

1'*!:.00+)5';!,7+!*1,1!5-!-+',!.4!,(!,7+!215'!*1,1!16B.5-5,5('!A-++!l!"=]?=!!&'!1**5,5('<!1!-+,!(0!$!DM`!-+)513!

4(5',!,(!4(5',!35'F-!0)(2!,7+!LEV!1)+!1**+*!,(!,7+!65)6.5,!(0!I5;.)+!"=$"$!,(!6(33+6,!2('5,()5';!*1,1!1'*!

-+,!9(3,1;+-<!+,6<!5'!,7+!1--(651,+*!*+956+-=!!!

!

Page 142: 2004 Ams Nim Paper Draft

AMS-02/RICH

!"#$$%!

iii?! Power Supplies

>7+! 215'! 0+1,.)+-! (0! ,7+! ,G(! *500+)+',! 4(G+)! -.443/! -/-,+2-! 1)+! -7(G'! 5'! >1:3+!"=Z=! ! T(,7!

-/-,+2-!.-+!"]e!5'4.,=!!>7+!75;7!9(3,1;+!-/-,+2!0()!,7+!J&KM!4)(95*+-!.4!,(!k%%!e!G+33!)+;.31,+*!1'*!

G5,7!9+)/!3(G!)5443+=!!>75-!9(3,1;+!5-!.-+*!,(!:51-!,7+!VD>-!1'*<!*.+!,(!,7+!*+4+'*+'6+!(0!,7+!;15'!G5,7!

,7+!9(3,1;+<!1!6(',)(3!1'*!2('5,()5';!-/-,+2!5-!)+B.5)+*=! !>7+!75;7!9(3,1;+!-/-,+2!5-!5243+2+',+*!5'!Y!

2(*.3+-!AJMe?=!!R167!2(*.3+!6(',15'-!,G(!9(3,1;+!+3+91,()-!5'!6(3*!)+*.'*1'6/!G5,7!1'!(.,4.,!9(3,1;+!

$!k%%!e=!!>7+!+3+91,()!0++*-!1!-+,!(0!Y%!0.33/!)+*.'*1',!Me!)+;.31,()-!G5,7!(9+)!6.))+',!4)(,+6,5('<!13-(!

3(61,+*!G5,75'! ,7+!2(*.3+=! !R167!(0! ,7+-+!(.,4.,-! -.4435+-!1! -+,!(0!Y!()!c!47(,(2.3,5435+)-=! !>7+!VD>!

671)16,+)5-,56-! A;15'! 9-=! 9(3,1;+<! +,6=?! 719+! :++'! 21,67+*! G5,75'! +167! -+,=! ! >7+! *+359+)+*! Me! 61'! :+!

)+;.31,+*!:+,G++'![c%!1'*!]c%!e=!!!

>7+!3(G!9(3,1;+!-/-,+2!0++*-!133!,7+!+3+6,)('56-!:.,!,7+!47(,(2.3,5435+)-=!!C-!-7(G'!5'!>1:3+!"=Z<!

,7)++!*500+)+',!9(3,1;+-!1)+!)+B.5)+*=!!>7+!m\<!!"!9(3,1;+-!0++*!,7+!1'13(;!0)(',#+'*!6754-!1'*!CLK-!1'*!

,7+!m\=\!9(3,1;+-!0++*!,7+!*5;5,13!6(',)(3!1'*!4)(6+--5';!41),=!!>7+!J&KM!3(G!9(3,1;+!-/-,+2!71-!]!:(1)*-!

3(61,+*!5'!,G(!:(8+-!ARJVL?!2(.',+*!('!,7+!215'!)1*51,()=!!R167!:(1)*!AI5;.)+!"=$""?!71-!1!415)!(0!LK#

LK! 6('9+),+)-<! 0()25';<! 1-! 0()! ,7+! 75;7! 9(3,1;+<! 1! 0.33/! )+*.'*1',! -/-,+2=! >7+-+! G+)+! *+9+3(4+*!

-4+65056133/! ,(! 2+,! CDE! )+B.5)+2+',-=! >7+/! 719+! 75;7! +00565+'6/! 1'*! 3(G! '(5-+=! ! K(3*! )+*.'*1',!

)+;.31,5('!(0!,7+!1'13(;!9(3,1;+-!5-!4+)0()2+*!1-!63(-+!1-!4(--5:3+!,(!,7+!1--(651,+*!3(1*-=!!!

!

High Voltage

_.,4.,!e(3,1;+ V(G+)!)+B.5)+*! J5443+!

[c%!,(!]c%!e! [!N! f!"%!2e

Low Voltage

_.,4.,!e(3,1;+ V(G+)!)+B.5)+*! J5443+!

m\=%!e! "%!N! f!c2e!

!"=%!e! [!N! f!c!2e!

m\=\!e! \c!N! fc%!2e!

!

Table 2.6: Characteristics of each Power Supply unit.

!

!!

Figure 2.122: DC-DC low voltage converter.

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AMS-02/RICH

! "#$$$

2.6.5 Tests with the RICH prototype

&'!()*+)!,(!9135*1,+!,7+!*+-5;'!(0!,7+!CDE#%"!J&KM<!1!4)(,(,/4+!AI5;.)+!"=$"\?!G5,7!1'!1))1/!(0!

k!8!$$!6+33-!-52531)!,(!,7(-+!(0!,7+!05'13!2(*+3!71-!:++'!6('-,).6,+*=!!>7+!4+)0()21'6+!(0!,75-!4)(,(,/4+!

71-!:++'!,+-,+*!G5,7!6(-256!2.('-!1'*<!5'!_6,(:+)!"%%"<!5,!G1-!4316+*!5'!1!:+12!(0!-+6('*1)/!5('-!1,!,7+!

KRJS!EVE!4)(*.6+*!:/!,7+!0)1;2+',1,5('!(0!1!V:!:+12=!!>7+!)5;5*5,/!-+,,5';-!0()!,7+!0)1;2+',-!('!,7+!

,)1'-4(),! 35'+! 133(G! 1'! +00+6,59+! -+3+6,5('! (0! ,7+! -+6('*1)/! 5('-!G5,7! -4+65056! 913.+-! (0! ,7+!21--! (9+)!

671);+!)1,5(=!!&'!41),56.31)<!:+12-!(0!4)(,('-!G5,7!)5;5*5,5+-!:+,G++'!c!^e!1'*!$\!^e!1'*!C@P!d!"!5('-!

G5,7! 1! )5;5*5,/! (0! Y%! ^e!G+)+! -+3+6,+*=! ! >7+! )5;5*5,5+-! G+)+! F'(G'!G5,7! 1'! 166.)16/! (0! $=cH=! ! >7+!

1';.31)!*59+);+'6+!(0!,7+!:+12!G1-!:+3(G!\!2)1*!-(!,71,! ,7+!-4)+1*!1,! ,7+!*+,+6,()!G1-!n$!62=!!T+12!

5',+'-5,5+-!G+)+!5'!,7+!)1';+!(0!$%"!,(!$%\!41),563+-!4+)!-4533=!

>(!19(5*!:16F;)(.'*-<!,7+!4)(,(,/4+!G1-!4316+*!5'-5*+!1!35;7,!,5;7,!6(',15'+)!1'*!,7+!-+,#.4!G1-!

6(243+2+',+*! G5,7! 1! -.44(),5';! -,).6,.)+! ,71,! 133(G+*! 671';+-! 5'! ,7+! )+31,59+! *5-,1'6+! :+,G++'! ,7+!

)1*51,()!1'*!,7+!*+,+6,5('!431'+=!!>7+!+84+)52+',13!-+,#.4!G1-!6(243+,+*!G5,7!,G(!-65',5331,5('!6(.',+)-!

,(!4)(95*+! ,7+!1!6(5'65*+'6+! ,)5;;+)!1'*!1!*(.:3+!2.3,5G5)+!4)(4(),5('13!6712:+)!ADNVK?!,(!2+1-.)+!

,7+! ,)1'-9+)-+! 6(()*5'1,+-!(0! ,7+!41),563+! ,)1O+6,()/!G5,7! 1! -.:253352+,+)! 166.)16/=! !>7+!2+1-.)+2+',-!

)+4(),+*!:+3(G!G+)+!4+)0()2+*!('!1!-1243+!(0!1:(.,!c!25335('!+9+',-!)+6()*+*!5'!1!Y!*1/!).'=!!>1:3+!"=[!

-7(G-!,7+!*500+)+',!-53561!C+)(;+3!)1*51,()-!.-+*!*.)5';!,7+!,+-,=!!!

!

!

!!

Figure 2.123: RICH prototype array of 9 x 11 cells (left), test beam set up (right).

Radiator n h (mm) d (mm) Stack

DRK! $=%\! Y""=c! "%! "!

DRK! $=%c! \[c=%! "%! "!

K&S! $=%\! Y""=c! \%! $!

K&S! $=%Y! Y""=c! \%! $!

!

Table 2.7: Different silica Aerogels studied in the CERN SPS Test Beam, with refractive index,

n, distance between the radiator and the detection plane, h, and sample thickness, d.

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AMS-02/RICH

!"#$$"!

>7+!)+6('-,).6,5('!13;()5,72-!0()!,7+!9+3(65,/!1'*!,7+!+3+6,)56!671);+!(0!,7+!5'6(25';!5('-!G+)+!

,7+! ('+-! *+9+3(4+*! 0()! ,7+! 05'13! *+,+6,()! G5,7! 25'()! 2(*50561,5('-! ,(! 166(.',! 0()! ,7+! 41),56.31)!

6('05;.)1,5('!(0! ,7+!+84+)52+',13!-+,!.4<! 5'!41),56.31)! ,7+!-.:-,5,.,5('!(0! ,7+!*1,1! 0)(2!DNVK!0()! ,71,!

0)(2!,7+!E5356('!>)16F+)=!!W-5';!,7+-+!,)16F!41)12+,+)-<!1!9+3(65,/!913.+!61'!:+!1--(651,+*!,(!+9+)/!-5';3+!

75,! 5'! ,7+! *+,+6,5('! 431'+=! ! >7+-+! 913.+-! 1)+! ;)(.4+*! 5',(! 63.-,+)-! 1'*<! 1-! *+,+)25'+*! :/! 1! *+65-5('!

13;()5,72<! ,7+! 2(-,! -5;'50561',! ('+! 5-! 1--(651,+*! ,(! ,7+! 41),563+! A-++! I5;.)+!"=$"Y?=! ! >7+! 9+3(65,/! 5-!

6(24.,+*!1-!,7+!2+1'!(0!,7+!6(',)5:.,5';!75,-<!+167!('+!G+5;7,+*!G5,7!,7+!6())+-4('*5';!-5;'13!5'!,+)2-!

(0!47(,(+3+6,)('-=! !I5'133/<! ,7+! ,)16F!1';.31)!41)12+,+)-!1)+!91)5+*! ,(!(4,525`+! ,7+!63.-,+)!-5;'50561'6+=!!

>7+!+-,521,+*!9+3(65,/!1'*!,7+!6(()*5'1,+-!(0!,7+!41),563+!1)+!.-+*!1-!5'4.,-!0()!,7+!671);+!)+6('-,).6,5('=!

>7+!13;()5,72!6(24.,+-<!('!1'!+9+',#:/#+9+',!:1-5-<!,7+!+84+6,+*!'.2:+)!(0!*+,+6,+*!47(,(+3+6,)('-!0()!

1!P!d!$!41),563+!ANexp?!G5,7!,7+!-12+!,)16F!41)12+,+)-!1'*!9+3(65,/!1-! ,7+!('+-!2+1-.)+*=!>75-!913.+! 5-!

6(241)+*!,(!,7+!16,.13!'.2:+)!(0!47(,(+3+6,)('-!+-,521,+*!0)(2!,7+!-5;'13!(0!,7+!2(-,!-5;'50561',!63.-,+)!

ANring?!1'*!,7+!671);+!(0!,7+!41),563+!671);+!5-!+-,521,+*!1- expringmeas NNZ @2 =!!!

>7+!2+1-.)+*!*5-,)5:.,5('!(0!671);+-!5'!,7+!:+12!5-!-7(G'!5'!I5;.)+!"=$"c!G7+)+!,7+!-,).6,.)+!(0!

5'*595*.13!5('!4+1F-!.4!,(!P!d!"Z!AI+?!5-!63+1)3/!95-5:3+!A4)(,('-!719+!:++'!-.44)+--+*?=!!>75-!-4+6,).2!

71-!:++'! 05,,+*! ,(!1! -.2!(0!^1.--51'!*5-,)5:.,5('-!1'*! 0)(2! ,7+5)!G5*,7-!G+!719+!+-,521,+*! ,7+!671);+!

)+-(3.,5('! 0()! +167!(0! ,7+! 5('-=! !>7+! )+-.3,-<! 6('-5-,+',!G5,7!G71,! 5-! +84+6,+*! 0)(2! ,7+! -52.31,5('<! 1)+!

-7(G'!5'!>1:3+!"=]!0()!,7+!*500+)+',!)1*51,()-!1'*!5'6(25';!5('-!(0!P!d!$<!"!1'*!Z=!

!

!!!!!! !

!!!!!! !!

Figure 2.124: A sample of Cerenkov rings detected with single, A/Z = 2, ion events.

!

Z=26Z=16

Z=2 Z=3 Z=6

Z~40

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AMS-02/RICH

! "#$$\

!!

Figure 2.125: Measured distribution of charges (Z>1) for the CIN n=1.03 radiator.

!

Radiator n Z = 1 Z = 2 Z = 6

DRK! $=%\! %=$kY!/!%=%%$! %=""[!/!%=%%$! %="c"!/!%=%%Y!DRK! $=%c! %=$]k!/!%=%%"! %="%$!/!%=%%$! %=""]!/!%=%%Z!K&S! $=%\! %=$k[!/!%=%%\! %=$kk!/!%=%%$! %="$[!/!%=%%Z!K&S! $=%Y! %=$k]!/!%=%%\! %=$k\!/!%=%%\! %="\"!/!%=%%[!

!

Table 2.8: Charge resolution for the different radiators and Z=1, 2 and 6 beams.

>7+! 166.)16/! 5'! ,7+! *+,+)25'1,5('! (0! ,7+! 9+3(65,/! 5-! +-,521,+*! 0)(2! ,7+! G5*,7! (0! ,7+! '()213!

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)1*51,()=!!!

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!"#$$Y!

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Figure 2.126: Velocity resolution for Helium nuclei from a fit to a

Gaussian distribution for the CIN n = 1.03 radiator.

!

Radiator n Z = 1 Z = 2

DRK! $=%\! %=[$!/!%=%"! %=Y]!!%=%$!

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!

Table 2.9: Velocity resolution (per mil) for the different radiators for protons and helium nuclei.

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! "#$$c

!!

Figure 2.127: Dependence of the velocity resolution on the charge

of the nuclei for the CIN n = 1.03 radiator.

!

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!

Front End electronics

PMT Calorimeter

HV divider

Shielding

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A(0/!,'0,!+.2,032?!%Uj!.9!,'(!(H(2,?!5?((!Q31G-(!"K$X"8K!!!

!

!!

70.8*'$!"6MF:$%134$'/'*.C$*';+&8)0+/"$$

!

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!"#$F"!

!!

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.

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! "#$FF

&'(! 021G*0-! -(?.*G,3.2! 0?! 0! 9G2+,3.2!.9! ,'(! (*(+,-.2! (2(-1JC!Q31G-(!"K$XFC! 3?!E(**! @(?+-3A(@!AJ!

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E0?! G?(@! E'3+'! ,0W(?! 32,.! 0++.G2,! .2*J! ,'(! /032! ?'.E(-! +'0-0+,(-3?,3+?! 50>(=C! @(>,'C! *0,(-0*! 02@!

*.213,G@320*!>-.93*(?8K! ! ;32+(! ,'(!A0+W1-.G2@! ,.! >.?3,-.2?!.9! (2(-1J!E(`! +./(?!/.?,*J! 9-./!>-.,.2?!.9!

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,'3?!>-.+(@G-(!E3,'!,'(!,(?,!A(0/!@0,0C!,'(!/./(2,G/!E0?!?/(0-(@!0++.-@321!,.!,'(!&-0+W(-!-(?.*G,3.2!

02@!,'(!/0,+'321!-(TG3-(/(2,!E0?!0>>*3(@!E3,'!0!+G,!)I>!p!<KUC!J3(*@321!0!90+,.-!.9!"<!3/>-.H(/(2,!32!

,'(!@3?+-3/320,3.2!>.E(-K!!!

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70.8*'$!"6ME:$3/.8&-*$*';+&8)0+/$S;"$'&'()*+/$'/'*.C"$$

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!"#$FV!

!!

70.8*'$!"6MP:$3/.8&-*$*';+&8)0+/$S;"$0/(0>'/)$-/.&'$<+*$6!F$Q'R$'&'()*+/;"$$

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.&%Uj B,D

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! "#$FX

!"#"#$ W'<'*'/(';$

B$D! QK!4(-H(**3!(,!0*KC!PG+*K!O2?,-K!02@!:(,'.@K!6!PBF!5"<<"8!$F"K!

B"D! [email protected]=!(,!0*KC!PG+*(0-!R'J?3+?!c!5R-.+K!;G>>*K8!66E!5"<<"8!$X]K!

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lK!6*+0-0L!(,!0*K!5,'(!6:;#<$!4.**0A.-0,3.28C!R'J?K!7(,,K!c!P9P!5"<<<8!$<_!!

lK!6*+0-0L!(,!0*K!5,'(!6:;#<$!4.**0A.-0,3.28C!R'J?K!7(,,K!c!PBM!5"<<<8!VV<K!

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!"#$%&!

2.8 Electronics '()! *+,!,-,.*)(/0.12!345!+61! *67,/! *+,!+08+!9,):();6/.,! *,.+/(-(80,1!<1,=! 0/!96)*0.-,!9+>10.1!

6/=! 0;9-,;,/*,=! *+,;! :()! <1,! 0/! -(?! @6)*+! ()A0*B! ! '08<),!"B$C&! 9)(D0=,1! 6/! (D,)D0,?! (:! *+,! 345!

,-,.*)(/0.1! ,-,;,/*1! 6/=! '08<),!"B$CE! 0/=0.6*,1! *+,! F353! 9)(D0=,=! 0/*,):6.,1! (/! *+,! G55B! ! 3! </0:0,=!

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6/=! ;(1*! 0;9()*6/*->2! A>! *+,! 9+>10.1! 8(6-1B! ! I6)*0.<-6)! ,::()*! +61! A,,/! ;6=,! *(! ,/1<),! *+6*! *+,! =6*6!

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(:!(9,)6*0(/B!!J+,!345!.),?!(9,)6*0(/1!9(1*!K3LMIN!?0--!6).+0D,!*+,!345!=6*6B!!4,,*0/8!*+,!.+6--,/8,1!

(:!0;9-,;,/*0/8!+08+!9,):();6/.,2!196.,!H<6-0:0,=!,-,.*)(/0.1!+61!A,,/!6!7,>!6.*0D0*>!(:!*+,!,/*0),!345!

.(--6A()6*0(/B!!!!!

!

!!

Figure 2.156: Overview of AMS-02 Electronics on the ISS and STS.

!

2.8.1 Interfaces !

31!0/=0.6*,=! 0/!'08<),!"B$CE2!F353!9)(D0=,1!*+),,!,-,.*)0.6-! 0/*,):6.,1!*(!345#O"!(/!*+,!G55P!

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0/*,):6.,1!:()!9(?,)!6/=!-(?!6/=!+08+!)6*,!=6*6!*)6/1:,)B!

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! "#$%E

!

!Figure 2.157: AMS electrical interfaces on ISS KJSR5P!J)6.70/8!6/=!S6*6!R,-6>!56*,--0*,2!

!!!!!!!!IMLLP!I6>-(6=!M9,)6*0(/1!6/=!L(/*)(-!L,/*,)2!4WLP!4(/0*()0/8!6/=!L(;;6/=NB!

!

i) Power Interface !

I(?,)!(/!*+,!G55!.(;,1!:)(;!*+,!,08+*!-6)8,!1(-6)!6))6>1B!345!?0--!+6D,!*?(!9(?,)!:,,=12!,6.+!

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*+01!-0;0*!A,0/8!,V*,/=,=!*(!"%OO!Z!:()!*+,!:0/6-!%O!;0/<*,1!(:!;68/,*!.+6)80/8B!!5*)0/8,/*!),H<0),;,/*1!

6),! 9-6.,=! (/! 345! A>! F353! 0/! *,);1! (:! 01(-6*0(/2! 8)(</=0/82! ,-,.*)(;68/,*0.! .(;96*0A0-0*>2! 0/)<1+!

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!"#$%\!

6--(.6*,=!*(!(9,)6*,!*+,!,-,.*)(/0.1B!!J+,!.(/D,)*,)1!9)(D0=,!*+,!:0)1*!01(-6*0(/!A6))0,)!6/=!=,-0D,)!6!1*6A-,!

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1*6*0(/B!!!

!

!!

Figure 2.158: AMS-02 Power Distribution System (PDS).

!

59,.06-!9)(D010(/!+61!A,,/!;6=,!*(!:,,=!*+,!.)>(;68/,*!6D0(/0.1!A(V!KL3]N!6/=!*+,!.)>(.((-,)1!

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! "#$%X

F353!9-6//0/8!0/=0.6*,1!*+6*!/(!</1.+,=<-,=!0/*,))<9*0(/1!?0--!(..<)!6/=!*+6*!:<--!9(?,)!?0--!A,!

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:()!6/!,V*,/=,=!0/*,)D6-B!!!

!

ii) Low Rate Data Link (LRDL) Interface !

J+,!QRSQ!01!A61,=!(/!*+,!4GQ!5JS!$CC%]!=<6-!1,)06-!A<12!?0=,->!<1,=!0/!60).)6:*B!!J+01!01!19-0*!

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!

!!

Figure 2.159: Practicing contingency EVA swap of AMS data cables at NBL.

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!"#$cO!

31!1+(?/!0/!'08<),!"B$&O2!*+01!*,-,;,*)>!=6*6!*+,/!9)(.,,=1!*+)(<8+!6!1,)0,1!(:!F353!</0*1!6/=!

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KJSR5N!*+)(<8+!*+,!Z+0*,!56/=1!f)(</=!L(;9-,V!KZ5fLN!*(!*+,!46)1+6--!596.,!'-08+*!L,/*,)!K45'LN!

6/=!*+,!d(+/1(/!596.,!L,/*,)!Kd5LNB!!Z0*+0/!*+,!U5!Q6A!(/!*+,!G552!*+,!61*)(/6<*!.),?!+61!6..,11!*(!*+01!

=6*6!D06!*+,0)!I()*6A-,!L(/*)(-!5>1*,;!KIL5N!-69*(91!6/=!D06!*+,!345!L),?!M9,)6*0(/1!I(1*!K3LMINB!!!

G/!*(*6-!345!01!6--(.6*,=!6A(<*!"O!e]0*1a1,.!(:!=6*6!A6/=?0=*+!(/!*+,!QRSQ2!?0*+!6/!,V9,.*,=!

=<*>!.>.-,!(:!<9!*(!EO`B!!J,/!+08+->!1<;;6)0[,=!A>*,1!9,)!1,.(/=!(:!.)0*0.6-!+,6-*+!=6*6!6),!*)6/1;0**,=!

?0*+!/,6)!*(!$OO`!=<*>!.>.-,B!!3-(/8!*+,!?6>!*+,!G55!.),?!6/=!F353!8)(</=!.(/*)(--,)1!.6/!;(/0*()!6*!

*+01!=6*6!6/=2!1+(<-=!*+,!/,,=!6)01,2!+6D,!*+,!:6.0-0*>!*(!011<,!6!:,?!7,>!.(;;6/=12!:()!,V6;9-,!*(!9<*!*+,!

,V9,)0;,/*!0/*(!6!1*6/=A>!1*6*,B!!G/!/(;0/6-!.(/=0*0(/12!6--!.(;;6/=1!()080/6*,!0/!*+,!IMLL!6/=!:(--(?!

*+,!0/D,)1,!96*+2!*+,!;6V0;<;!.(;;6/=!)6*,!A,0/8!6A(<*!$!eA0*a1,.(/=B!

31!.(;;6/=0/8!6/=!*,-,;,*)>!6),!.)0*0.6-! *(! *+,!(9,)6*0(/!(:! *+,!,V9,)0;,/*!6/=!61! *+,!F353!

9)(D010(/1!:()!96>-(6=1!6),!/(*!:6<-*!*(-,)6/*2!1<A1*6/*06-!,::()*!+61!A,,/!;6=,!*(!0;9-,;,/*!6!96)6--,-!1,*!

(:!=6*6!96*+1!(D,)!*+,!TRSQ!:()!A(*+!;(/0*()0/8!6/=!.(;;6/=0/8!(:!345B!!!

!

!!

Figure 2.160: Monitoring and Command Data Flow over both the LRDL and HRDL.

J+,!</1+6=,=!F353!1<99-0,=!</0*1!6),!=,:0/,=!0/!*+,!*,V*B!

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AMS-02/Electronics

! "#$c$

iii) High Rate Data Link (HRDL) Interface !

J+,!TRSQ!01!*+,!;60/!=6*6!.(/=<0*!(<*!(:!345B!!G*!01!A61,=!(/!6!F353!19,.0:0.!0;9-,;,/*6*0(/!

(:!:0A,)!(9*0.!.(;;</0.6*0(/1B!!J+,!-0/7!.6/!;(D,!=6*6!(/!*+,!G55!6*!19,,=1!<9!*(!XO!4]0*a1,.2!6/=!*+,!

)6=0(!=(?/!-0/7!1<99()*1!<9!*(!c%!4A0*a1,.2!6860/!?0*+!6/!6*!A,1*!=<*>!.>.-,!(:!EO`B!!M:!*+01!345!+61!

A,,/!6--(.6*,=!6/!()A0*!6D,)68,!(:!"!4A0*a1,.B!!Z0*+0/!3452!*+,!=6*6!01!.(--,.*,=!A>!*+,!=6*6!6.H<010*0(/!

KS3gN!1>1*,;!*(!6!A<::,)!?0*+0/!*+,!d4SL1B!!31!:()!*+,!QRSQ2!,6.+!(:!*+,!:(<)!d4SL!01!.(//,.*,=!*(!

*+,!TRSQ!6/=!6!.6A-,!1?69!=<)0/8!@Y3!6D(0=1!6!9(110A-,!10/8-,!9(0/*!(:!:60-<),B!!M/!*+,!TRSQ!*+,!=6*6!

:-(?1! (D,)! *+,! 96*+1! 1+(?/! 0/! '08<),!"B$&$B! !3! 7,>! ,-,;,/*! 0/! *+01! 96*+! 01!3LMI2!?+,),! *+,! =6*6! 01!

6).+0D,=!(/!=0171B!3LMI!?0--!A,!;(</*,=!0/!6/!@V9),11!R6.7!0/10=,!(:!6/!G55!5*6/=6)=!I6>-(6=!R6.7!

KG5IRNB!!M/!*+,!8)(</=!*+,!=6*6!01!)(<*,=!*(!*+,!345!IMLL!6/=!5.0,/.,!M9,)6*0(/!L,/*,)B!!!

Figure 2.161: AMS Science data flow over the of High Rate Data Link.

!!!!!!!!!J+,!</1+6=,=!F353!1<99-0,=!</0*1!6),!=,:0/,=!0/!*+,!*,V*B!

!

2.8.2 Subdetector Electronics !

J6A-,!"B$O!1<;;6)0[,1!*+,!,-,.*)(/0.1!),H<0),;,/*1!(:!*+,!=0::,),/*!=,*,.*()1!=,1.)0A,=!,6)-0,)!0/!

*+01!.+69*,)B!!J+,!JRS!),H<0),1!*+,!861!860/!*(!A,!.6),:<-->!.(/*)(--,=B!!J+,!*0;,!(:!:-08+*!1>1*,;!),H<0),1!

),-6*0D,!*0;0/8!6..<)6.>!(:!$OO!90.(1,.(/=12!*+,!10-0.(/!;0.)(1*)09!*)6.7,)!),H<0),1!108/6-1!61!1;6--!61!6!

:,?!:,;*(.(<-(;A1! *(!A,!;,61<),=!?0*+!6!108/6-! *(!/(01,!1<99),110(/!(:!$OCB! !J+,!RGLT!),H<0),1! *+6*!

10/8-,!D010A-,!9+(*(/1!A,!;,61<),=B!!J+,!@L3Q!),H<0),1!6!?0=,!=>/6;0.!)6/8,!(:!&O2OOOB!!G/!*(*6-!*+,),!

6),!h%OO2OOO!1,96)6*,!1<A=,*,.*()!=,*,.*()!.+6//,-1!9)(=<.0/8!%BE!4]0*!(:!=6*6!:()!,D,)>!*)088,)B!

!

!

!

!

!

!

Page 174: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$c"!

Subdetector!Critical

Requirement!Channels!

Raw

Kbits!

U: TRD! f61!860/! C2"c\! \c! !

S: ToF+ACC! $OO!91! c\ici\! cX! !

T: Tracker! :,?!:L! $X&2&O\! %2$c&! !

R: RICH! 50/8-,!!! &\Oi$&i"! %c\! !

E: ECAL! $P&O2OOO! %"ciKci"j$N! cE! !

H Raw Kbits/event * Event Rate! %2&Ec! i!$!"!e+[!

!!!= Total Raw Data Rate :! ~7 Gbit/sec!

Table 2.10: Subdetector electronics requirements and raw data volumes.

J+(<8+! *+,! =,*60-,=! ),H<0),;,/*1! 0;9(1,=! A>! *+,! 9+>10.1! 6),! =0::,),/*! :()! ,6.+! (:! *+,!

1<A=,*,.*()12! 6!</0:0,=!699)(6.+!+61!A,,/!6=(9*,=! :()! *+,0)!,-,.*)(/0.1B! !J+01!699)(6.+! 01!A61,=!(/! *+,!

1<..,11:<-!,V9,)0,/.,!860/,=!?0*+!*+,!345#O$!,/80/,,)0/8!:-08+*2!<9=6*,=!:()!/,?!*,.+/(-(80,12!:()!*+,!

1<A=,*,.*()1!?+0.+!?,),! /(*! 0/1*6--,=! (/!345#O$! 6/=! :()! *+,! *08+*! ),1(<).,! ),H<0),;,/*1! A(*+! (/! *+,!

8)(</=! K*0;,2!;(/,>2!;6/9(?,)N! 6/=! (/! ()A0*! K?,08+*2! 9(?,)2! =6*6! )6*,NB! ! J+01! 699)(6.+! 01! 1+(?/! 0/!

'08<),!"B$&"B!!3/6-(8!108/6-1!:)(;!*+,!=,*,.*()1!,/*,)!6!=,*,.*()!19,.0:0.!399-0.6*0(/!59,.0:0.!G/*,8)6*,=!

L0).<0*! K35GLN! 6/=! 6),! :0)1*! 1+69,=2! 6/=! *+,/! +,-=! 0/! ),19(/1,! *(! 6! *)088,)2! *+,! *)088,)! +6D0/8! A,,/!

8,/,)6*,=! <10/8! 108/6-1! :)(;! *+,! =,*,.*()1! 61! 1+(?/! 0/! '08<),!"B$&%B! ! J+,! +,-=! 108/6-1! 6),! *+,/!

;<-*09-,V,=! ?0*+! *+,! 35GLB! ! J+,1,! 6),! ;(</*,=! .-(1,! *(! *+,! =,*,.*()! ,-,;,/*1B! ! ],:(),! ()! 6:*,)!

=080*0[6*0(/2!*>90.6-->!?0*+!6/!3SL2!*+,!(<*9<*!01!*+,/!1,/*!(D,)!6!.6A-,!0/*(!6!LSI!K.(;;(/!=080*6-!96)*N!

6/=! A<::,),=! 0/*(! ;,;()0,1B! ! Z0*+! ;<-*09-,V0/82! ,6.+! LSI! .(--,.*1! =6*6! :)(;! <9! *(! $OOO! =0::,),/*!

1<A=,*,.*()! 108/6-1B! !3!</0:0,=!699)(6.+!?61!6-1(!699-0,=! *(! *+,!;(/0*()0/8!6/=!.(/*)(-! K4WLN!(:! *+,!

1<A=,*,.*()! 96)6;,*,)1! 6/=! *(! *+,0)! 9(?,)! 1<99-0,1B! ! 31! =01.<11,=! A,-(?2! 6--! (:! *+,! .(;9(/,/*1! 6/=!

.0).<0*1!<1,=! 0/! *+,1,!</0:0,=!699)(6.+,1!+6D,!8(/,! *+)(<8+!6! )08()(<1!9)(.,11! *(!,/1<),! *+6*! *+,>!?0--!

;,,*!*+,!9,):();6/.,!),H<0),;,/*1!6/=!(9,)6*,!),-06A->!0/!(<*,)!196.,B!!!

!

!

!

Figure 2.162: Unified approach to subdetector electronics for DAQ,

Monitoring and Control (M&C) and power.

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AMS-02/Electronics

! "#$c%

!

Figure 2.163: Fast (FT) and Level-1 (LV1) Trigger Scheme (FF - flip flop).

!

2.8.3 DAQ and Trigger Electronics !

J+,!9+>10.1!=6*6! :-(?!0/! *+,!,-,.*)(/0.1! 01!=)0D,/!A>! *+,! *)088,)!1>1*,;!1+(?/!0/!'08<),!"B$&%B!!

J+01!1>1*,;!),.(8/0[,1!?+,/!6!.+6)8,=!96)*0.-,!+61!9611,=!*+)(<8+!*+,!=,*,.*()!A61,=!(/!*+,!.(0/.0=,/.,!

(:!:61*!108/6-1!:)(;!*+,!*0;,!(:!:-08+*!1.0/*0--6*()1B!!G*!*+,/!-((71!6*!:61*!108/6-1!:)(;!*+,!3LL!6/=!@L3Q!

*(! .+,.7! *+6*! *+,! 96)*0.-,! .-,6/->! 9611,=! *+)(<8+! *+,! =,*,.*()B! ! G/! 6==0*0(/! *(! .+6)8,=! 96)*0.-,12! +08+!

,/,)8>! 86;;6! )6>1! 6),! 6-1(! *)088,),=! ?+,/! *+,>! 960)! 9)(=<.,! ,-,.*)(/1! 0/! *+,! JRSB! ! U/.(/D,)*,=!

9+(*(/1! 6A(D,! $!f,Y! 6),! 6-1(! *)088,),=! A61,=! (/! 1*6/=#6-(/,! 96**,)/! ),.(8/0*0(/! 0/! *+,! @L3Q!?+0.+!

),k,.*1!*+,!9)0;6)>!A6.78)(</=!(:!(::!6V01!-(?!,/,)8>!9)(*(/1B!!J+,!*(*6-!*)088,)!)6*,!01!,1*0;6*,=!:)(;!*+,!

;,61<),;,/*1! 9,):();,=! A>! 345#O$! *(! D6)>! :)(;! "OO! *(! "OOO!T[2! =,9,/=0/8! (/! *+,! 8,(;68/,*0.!

-6*0*<=,B! !J+,!,-,.*)(/0.1!1>1*,;!01!A,0/8!.(/1,)D6*0D,->!=,108/,=!*(!9,):();!9),.010(/!9+>10.1!6*! *?0.,!

*+,1,!)6*,1B!!!

J,.+/0.6-->2!*?(!LSI1!6),!-(.6*,=!(/!(/,!VSR!A(6)=!K1,,!'08<),!"B$&cN2!?+,),!Vl@2!R2!52!J2!U!

:()!*+,!=0::,),/*!1<A=,*,.*()1B!!'()!*+,!RGLT!6/=!J)6.7,)2!VlR2!J2!*+,!*?(!LSI!6),!0/=,9,/=,/*B!!'()!*+,!

@L3Q2!5.0/*0--6*()1!6/=!JRS2!Vl@2!52!U2!*+,!*?(!LSI!6),!0/!.(-=!),=</=6/.>B!!G/!6--!.61,12!(/.,!*+,!)6?!

=6*6! 01! 1*(),=! 0/*(! ;,;()>2! *+,! :(--(?0/8! S3g! .0).<0*)>! 01! *+,! 16;,! :()! 6--! *+,! 1<A=,*,.*()1B!!

31>/.+)(/(<1->!?0*+!1<A1,H<,/*!*)088,)12!*+,!=6*6!?0*+0/!6!LSI!01!),=<.,=!<10/8!6!1<A=,*,.*()!19,.0:0.!

6-8()0*+;!0/!6!=080*6-!108/6-!9)(.,11()!KS5IN!6/=!),A<::,),=B!!Z+,/!),1(<).,1!6),!6D60-6A-,!*(!),.,0D,!0*2!

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.0).<0*! -(.6*,=!(/! 6! dGF'!A(6)=2! ),.,0D,1! =6*6! :)(;!<9! *(! "c!LSIB! !J+,!LSSL! 01! 0/! :6.*! 6!LSI!?0*+!

;(=0:0,=!:)(/*!,/=!6/=!-6)8,)!;,;()0,1B!!!

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*+,! *(9! -,D,-!LSSL1! -(.6*,=!(/!dGFd!A(6)=12! .(--6*,=2!A<::,),=!6/=! 0/! *<)/!9611,=! 0/*(!6! d4SLB! !J+,!

d4SL!),.,0D,1!*+,!.(;9-,*,!,D,/*!6/=!6/6->1,1!0*!*(!,/1<),!*+6*!0*!;08+*!.(/*60/!0/*,),1*0/8!9+>10.1!6/=!

6-1(!*(!;(/0*()!*+,!=,*,.*()!9,):();6/.,B!!J+,!1,-,.*,=!,D,/*1!6),!*+,/!A<::,),=!6/=!1,/*!(<*!*+,!TRSQ!

?+,/!0*!A,.(;,1!6D60-6A-,B!!!

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'08<),1!"B$&c!6/=!"B$&CB!!

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AMS-02/Electronics

!"#$cc!

')(;!J6A-,!"B$O2!*+,!9,67!)6?!=6*6!)6*,!01!E!f]0*a1,.B!!J+,!,V*,/10D,!=6*6!),=<.*0(/!9,):();,=!0/!

96)6--,-!0/!*+,!"\c!:)(/*!,/=!S3g!;(=<-,1!.(;A0/,=!?0*+!A<::,)0/8!*+)(<8+!(<*!*+,!S3g!*),,!6/=!0/!*+,!

d4SL2! 9-<1! 6==0*0(/6-! ,D,/*! :0-*,)0/8! 0/! *+,! d4SL2! 6--(?1! *+01! )6*,! *(! A,! ),=<.,=! *(! *+,! 6--(.6*,=!

"!4]0*a1,.!()A0*!6D,)68,B!!!

!

2

22

2

2

22

2

from

Subd

etec

tor’

Fro

nt!

Ends

Front!EndDAQ Modules

284 x 1(2) 1 x 4Top!Level

CDDC ComputersMain DAQ

1 x 4

16

4 x 2 SDR, 1x2 JLV1,Lowest!Level CDDC,

14 x 2

4

4

4

4

xDR

xDR

xDR

xDR

xDR

xDR

xDR

xDR

JINJ JMDC

JINF

JINF

JINF

JINF

Data Commands

Commands

Data Commands Data "Final" Data

!!

Figure 2.164: The DAQ tree. The number of redundant links at each level is indicated.

!24 4 4

2

from

Subd

etec

tor’s Fro

nt!

End

J422

JF

OM

JF

OM

CDDCTop!Level Main DAQ

ComputersFront!End

DAQ ModuleLowest!Level

CDDC JHIF

224

JMDC

JMDC

JMDC

JMDC

CDDC

CDDC

JINF

JINJ

xDR

JINJ

JINJ

JINJ

RS422Data

CommandsCommands

DataCommands

HRDL

HRDL

Data

!!

Figure 2.165: The DAQ tree. The number of redundant nodes at each level is shown.

!

J+,!d4SL!01!A61,=!(/!6!9(?,):<-!),.,/*!;0.)(9)(.,11()2!*+,!G]4!I(?,)IL!ECO2!0;9-,;,/*,=!

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L3F! A<1! :()!;(/0*()0/8! 6/=! .(;;6/=! *)6/1:,)12! *(! *+,!S3g!345Z0),! -0/71! 6/=! *(! *+,!TRSQ! 6/=!

QRSQ!6/=! *+,!,H<0D6-,/*!=6*6! -0/71! :()! *+,! 1+<**-,B! !31! :()! *+,! 1<A=,*,.*()! ,-,.*)(/0.12! *+,! d4SL!6/=!

9,)09+,)6-1!+6D,!9611,=!*+)(<8+!6/!,V*,/10D,!196.,!H<6-0:0.6*0(/!9)(.,11B!!!

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AMS-02/Electronics

! "#$cC

2.8.4 AMS Crew Operations Post (ACOP) !

3LMI! 01! 6 .(;9<*,)! *+6*! 01! A,0/8! 19,.0:0.6-->!=,108/,=! :()!345#O"B! ! G/! :-08+*2! *+,!=01*0/.*0(/!

A,*?,,/!3LMI!6/=!*+,!(*+,)!,-,.*)(/0.1!.(#-(.6*,=!?0*+!345!01!*+6*!3LMI!01!-(.6*,=!0/10=,!*+,!U5!-6A!

;(=<-,!(:!*+,!G55!6/=!.6/!A,!6..,11,=!A>!*+,!61*)(/6<*!.),?2!61!1+(?/!0/!'08<),!"B$&&2!?+,),61!*+,!(*+,)!

:-08+*!,-,.*)(/0.1!01!-(.6*,=!(<*10=,2!</=,)!D6.<<;2!/,V*!*(!*+,!=,*,.*()1!(/!*+,!5%!*)<11!(:!G55B!!J+,!;60/!

:</.*0(/!(:!3LMI!01!*(!6).+0D,!*+,!=6*6!:)(;!*+,!,V9,)0;,/*!6))0D0/8!:)(;!345#O"!(/!*+,!TRSQ!:0A,)!

(9*0.!=6*6!-0/7B!!G/!6==0*0(/2!0*!6--(?1!*+,!.),?!*(!;(/0*()!6/=2!0:!/,.,116)>2!.(;;6/=!*+,!,V9,)0;,/*2!61!

A(*+!(/!3LMI!6/=!?0*+0/!*+,!345#O"!d4SL1!A0#=0),.*0(/6-!:0A,)!(9*0.!-0/71!6),!0;9-,;,/*,=B!!!

3LMI! 01! :(),1,,/! *(!A,!A61,=!(/!6!L(;96.*ILG! :();6*! 1>1*,;! 0/!.(;;(/!?0*+! *+,! !345#O"!

d4SL! 1>1*,;1B! ! 3! .(/.,9*<6-! =,108/! 01! 1+(?/! 0/! '08<),!"B$&EB! ! 3LMI! ?0--! .(/*60/! 6! 10/8-,! A(6)=!

.(;9<*,)!.(;96)6A-,!*(!*+6*!(:!*+,!d4SL!A<*!?0*+!,V*,/=,=!;,;()>!6/=!(/#A(6)=!9,)09+,)6-1B!3LMI!

),H<0),1!6!.<1*(;!=,D,-(9,=!0/*,):6.,!:()!*+,!T08+!R6*,!S6*6!Q0/7!KTRSQN!6/=!(*+,)!9,)09+,)6-!=,D0.,12!

0/.-<=0/8! @*+,)/,*! 0/*,):6.,1! *(! 1<99()*! *+,!4,=0<;! R6*,! S6*6! Q0/7! K4RSQN2! 6! .(;96.*! :-61+! KL'N!

.6))0,)!*(!1*(),!*+,!(9,)6*0/8!1>1*,;!6/=!9)(8)6;1!6/=!=080*6-!0/9<*#(<*9<*!6/=!D0=,(!.6)=1!KSGM2!Yf3N!

?+0.+! .(//,.*! *(! 6! 10;9-,! 9<1+! A<**(/! 0/*,):6.,! 6/=! 6! :-08+*! H<6-0:0,=! QLS! 1.),,/B! ! 3LMI!?0--! 6-1(!

.(/*60/!:(<)!,V.+6/8,6A-,!+6)=!=0171!<1,=!*(!6).+0D,!*+,!=6*6!6/=!*+,!/,.,116)>!0/*,):6.,1B!!!

G/!6==0*0(/!*(!*+,!3LMI!1>1*,;!*+,),!?0--!A,!1*(?68,!A68!1,/*!*(!G55!*+6*!?0--!.(/*60/!6==0*0(/6-!

+6)=!=)0D,1!*+6*!.6/!A,!,V.+6/8,=!?0*+!*+,!+6)=!=)0D,1!0/!3LMIB!!')(;!*0;,!*(!*0;,!*+,!61*)(/6<*1!?0--!

9,):();!*+01!,V.+6/8,!,/6A-0/8!3LMI!*(!),.()=!6--!(:! *+,!345#O"!=6*6!(/*(!:),1+!+6)=!=)0D,1B! !@V6.*!

+6)=! =017! .696.0*>! 01! </=,)! 1*<=>2! A<*!?0*+(<*! .),?! 0/*,)D,/*0(/!3LMI! 1+(<-=! A,! 6A-,! *(! 6).+0D,! *+,!

(<*9<*!(:!345!:()!6!;(/*+B!!Z0*+!=017!1?6990/8!*+01!,V*,/=1!*(!10V!;(/*+1B!!M/.,!),.()=,=2!*+,!=6*6!?0--!

/(*!A,!(D,)?)0**,/m!)6*+,)!0*!?0--!A,!*)6/19()*,=!*(!*+,!8)(</=!61!6!9,);6/,/*!6).+0D,B!

!

!!

Figure 2.166: Typical ACOP location Inside the US Lab onboard the ISS.

typical ACOP

location

Page 178: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$c&!

!!

Figure 2.167: Conceptual design of ACOP.

!

345! 01! ,V9,.*,=! *(! 9)(=<.,! =6*6! 6*! "!4A0*a1,.! 6D,)68,2! ()! $j!f]>*,a+(<)B! ! J+01! .(/*0/<,1!

"c!+(<)1!9,)!=6>2!E!=6>1!9,)!?,,72!:()!*+,!*+),,!>,6)!;0110(/!=<)6*0(/B!!46/680/8!*+01!=6*6!:-(?!*+)(<8+!

*+,!G55!1>1*,;1!?0--!),H<0),!1<A1*6/*06-!A<::,)0/8!6/=!0/*,)6.*0(/!6/=!9-6.,!6!1<A1*6/*06-!-(6=!(/!*+,!G55!

1>1*,;1B!!Z+0-,!*+,!G55!+08+!)6*,!=6*6!1>1*,;1!+6D,!A,,/!=,;(/1*)6*,=!*(!(9,)6*,!*(!19,.0:0.6*0(/2!*+,>!

+6D,!/(*!A,,/!<1,=!6*!+08+!D(-<;,!.(/*0/<(<1->!:()!*+,!?,,712!;(/*+12!>,6)1!*+6*!345!),H<0),1B!!3LMI!

?0--! ,/1<),! *+6*! *+,! .)0*0.6-! (<*9<*!(:!3452! *+,! 1.0,/.,! =6*62! 01! .69*<),=! 6/=! 6..,110A-,! 61! 1,.<),->! 61!

9(110A-,B!!!

3LMI! 6-1(! 9)(D0=,1! 6! :-,V0A-,! 6/=! 1*)608+*! :()?6)=! ;,6/1! :()! *+,! 61*)(/6<*1! *(! 0/*,)6.*! ?0*+!

345B! !M/,!(:!;(1*! 0;9()*6/*! ),1(<).,1!(/! G55! 012! (:! .(<)1,2! *+,! .),?B! !J+01!;67,1! *+01! ,/D0)(/;,/*!

.(;9-,*,->!</0H<,B!!G/!()=,)!*(!96)*0.096*,2!*+,!61*)(/6<*!/,,=1!6!;,6/1!*(!;(/0*()!6/=!.(/*)(-!345#O"B!!

L,)*60/!7,>!(9,)6*0(/12!-07,!;68/,*!.+6)80/82!),H<0),!*+,!61*)(/6<*1!*(!.(/*0/<(<1->!;(/0*()!345#O"!6/=!

A,!9),96),=!*(!,V,)*!.(/*)(-B!!3LMI!01!6!:-,V0A-,!6/=!9(?,):<-!*((-!*(!;(/0*()!6/=!.(/*)(-!345#O"B!

3LMI!6-1(!9)(D0=,1!6/!6-*,)/6*,!.(;;6/=!96*+!*(!345B!!J+,!=,108/!(:!*+,!G55!6D0(/0.1!1>1*,;1!

+61! /(! *(-,)6/.,! :()! 6/>! :60-<),! (:! 1,)D0.,1! ?0*+! ),86)=! *(! 96>-(6=1B! ! J+,),! 01! 6! 10/8-,! 96*+! :()!

.(;;6/=0/8! 6/=!;(/0*()0/8! 6! 96>-(6=B! ! G:! *+01! :60-1! *+,),! 01! /(! 6-*,)/6*0D,! A<*! *(! ),960)! *+,! 0/*,):6.,B!!

J+01!01!*+,!8),6*!*+0/8!6A(<*!*+,!196.,!1*6*0(/m!*+,),!01!1(;,(/,!*+,),!*(!:0V!*+0/81B!!T(?,D,)!*+,!*0;,!*(!

0;9-,;,/*! 6! ),960)! 01! D,)>! +08+B! ! @D,/! *+,! 10;9-,1*! ),960)! .6/! *67,1! ?,,71! ()! ;(/*+1! n! .,)*60/->! 6/!

0;9)(D,;,/*!(D,)!/,D,)2!?+0.+!01!*+,!6-*,)/6*0D,!:()!/(/#;6//,=!1>1*,;1B!!50/.,!*+,!1<9,)!:-<0=!+,-0<;!

?0--!A,!A(0-0/8!6?6>!?+0-,! ),960)1!6),!6::,.*,=2! 108/0:0.6/*!=6*6!86*+,)0/8!.696.0*>!?(<-=!A,! -(1*! 0/! *+,!

,D,/*!(:!6/>!:60-<),B!!3LMI!6::()=1!6/!6-*,)/6*,!96*+!:)(;!?+0.+!.(;;6/=1!.6/!A,!1,/*!:)(;!*+,!8)(</=!

*(!345#O"B!!!

!

!

!

!

Fan!Boards!

Display!Power!Supply!

cPCI!Card!Cage!

SwappableHard Drives

Connectors!

Push!Buttons!

Single Board Computer

CF VGA DIO

HRDL E’net

Page 179: 2004 Ams Nim Paper Draft

AMS-02/Electronics

! "#$cE

2.8.5 Particle Physics Electronics in Space !

J6A-,!"B$$! 1<;;6)0[,1! *+,! .+6--,/8,1! :6.,=! A>! *+,! 345! .(--6A()6*0(/! 0/! 9),96)0/8! 96)*0.-,!

9+>10.1!,-,.*)(/0.1!:()!<1,!0/!196.,B!!J+,!7,>!9(0/*!:()!345#O"!,-,.*)(/0.1!01!=,)0D,=!:)(;!(<)!,V*,/10D,!

A6.78)(</=!0/!0/1*)<;,/*6*0(/!(:!+08+!,/,)8>!9+>10.1!=,*,.*()1!6/=!(<)!,V9,)0,/.,!?0*+!345#O$!6/=!01!

)08()(<1->! *,1*,=! 6--! *+,!?6>! :)(;! *+,! =,108/! 9)(*(*>90/8! 6/=! .(;9(/,/*! 1.),,/0/8! *+)(<8+! A(V! -,D,-!

6..,9*6/.,!*,1*1B!!!

345!+61!D61*->!;(),!=,;6/=0/8!),H<0),;,/*1!*+6/!*+(1,!:()!<1<6-!196.,!,-,.*)(/0.12!0/!*,);1!(:!

*+,! 9,):();6/.,2! .(;9-,V0*>! 6/=! ),1(<).,1! K9(?,)2! ?,08+*2! 1.+,=<-,NB! ! J+,! ),H<0),;,/*1! (:! ,6.+!

1<A1>1*,;!+6D,! A,,/! 1*<=0,=! 0/! =,*60-! 6/=! 6/! (9*0;0[,=! 9)(8)6;! *(!;,,*! *+,1,! ),H<0),;,/*1! +61! A,,/!

0;9-,;,/*,=B! ! '()! ,V6;9-,2! 0/! *+,! L)>(;68/,*! 3D0(/0.1! ](V! KL3]N! 0*! 01! /(*! 9(110A-,! *(! .(//,.*!

.(;9-,*,->!),=</=6/*!1>1*,;1!*(!*+,!;68/,*2!1(!+,6D>!<1,!01!;6=,!(:!196.,!8)6=,!.(;9(/,/*1B!!!

!

Challenge Solution

5*6*0.!Q(6=1! cOj$Oj$O8!

Y0A)6*0(/! &B%!8);1!

S,9),11<)0[6*0(/! $!*(!O!A6)!a!"!;0/!

4,.+6/0.6-!S,108/!W!J,1*!

o,)(!f! '-(6*,)1! L(/:();6-!.(6*0/8!

Y6.<<;! F(!L(/D,.*0(/! Z61*,!T,6*!L(/=<.*0(/!

J+,);6-!!cO2!j\O!,L!5<)D0D6-!!%O2!jCO!,L!M9,)6*0(/!

I6)*1!5,-,.*0(/2!4,.+B!!

!!!S,108/!W!J,1*0/8!

R6=06*0(/! h!$!eR6=!a>,6)! JGS!J,1*0/8!

T,6D>!G(/! Q6*.+!U912!]0*!'-091! ],6;!J,1*0/82!@))()!SaL!

3*(;0.!M! @*.+0/8!

5(-6)!UY! 380/8!

46*,)06-!5,-,.*0(/!W!4,.+6/0.6-!

5+0,-=0/8!

44aMS! I</.*<),1! 4(),!5+0,-=0/8!

@4L! F(01,2!R,H<0),;,/*1! f)(</=2!'0-*,)2!5.),,/!

468B!'0,-=! U9!*(!h!COO!f6<11! J,1*0/82!I-6.,;,/*!

3..,11! F(/,!:()!%j!>,6)1! R,-06A0-0*>2!R,=</=6/.>2!J,1*0/8!

!

Table 2.11: Challenges and solutions in flying state of the art electronics in low Earth

orbit. Design and production follow processes validated with AMS-01.

!

G/! .(/*)61*! *+,! S3g! 1>1*,;! 9)0;6)0->! <1,1! +08+! 8)6=,! .(;;,).06-! .(;9(/,/*1! 6/=! 6.+0,D,1!

),-06A0-0*>!A>!0/*,).(//,.*0/8!),=</=6/*!,-,;,/*1B!!J(!,/1<),!*+6*!*+,1,!?0--!?()7!0/!196.,2!6!9)(.,11!+61!

A,,/! =,D,-(9,=! -,6=0/8! :)(;! 0*,)6*0(/1! (:! .0).<0*! =,108/! 6/=! .(;9(/,/*! 1,-,.*0(/! *+)(<8+!;,.+6/0.6-!

=,108/!6/=!;6*,)06-! 1,-,.*0(/! *(! *+,!9)(=<.*0(/2!H<6-0*>!611<)6/.,!6/=!196.,!H<6-0:0.6*0(/!(:!6!1,)0,1!(:!

;(=,-1B! !31! 0/=0.6*,=! 0/!'08<),!"B$&\2!.6/=0=6*,!.(;9(/,/*1!6),!<1,=! *(! 0;9-,;,/*!9)(*(*>9,!.0).<0*1B!!

J+,1,! 6),! *+,/! .(;A0/,=! 0/*(! :</.*0(/6-->! ,H<0D6-,/*! ,/80/,,)0/8! ;(=,-1!K@4NB! ! J+,! @4! 6),! *+,/!

),0;9-,;,/*,=!<10/8!+08+!),-06A0-0*>!.(;9(/,/*1!0/!*(!6!1,)0,1!(:!H<6-0:0.6*0(/!;(=,-1!Kg4N2!?+0.+!9611!

*+)(<8+!6!1,)0,1!(:! *,1*1! 0/.-<=0/8!D0A)6*0(/!6/=! *+,);6-!.>.-0/8!6*!A(6)=! -,D,-!Kg4$N!6/=!6-1(! *+,);6-!

D6.<<;!6/=!,-,.*)(;68/,*0.!.(;96*0A0-0*>!K@4LN!6*!A(V!-,D,-!Kg4"NB!!'08<),1!"B$&X!*(!"B$E$!1+(?!*+,!

g4"!D,)10(/!(:!*+,!.)6*,!.(/*60/0/8!*+,!d4SL!</=,)8(0/8!*+,1,!*,1*1B!!J+,!g4"!A(6)=1!6),!6-1(!<1,=!*(!

.(;9-,*,->!0)(/!(<*!6--!70/71!0/!*+,!9)(=<.*0(/!9)(.,11B!!J+,!:-08+*!;(=,-1!6/=!:-08+*!196),1!K'42!'5N!6),!

9)(=<.,=!6/=!H<6-0:0,=!?0*+!D0A)6*0(/!*+,);6-!.>.-0/8!6/=!*+,);6-!D6.<<;!*,1*1! *(! *+,!;0/0;<;!-,D,-1!

),H<0),=!,/1<)0/8!*+6*!,6.+!9,):();1!61!*+,!1<..,11:<-!g4"!</0*1B!!!

Page 180: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$c\!

Figure 2.168: AMS-02 Process for producing space qualified electronics.

Figure 2.169: The JMDC crate under thermal cycling tests, with the test profile

(10 cycles are performed before vibration and 5 afterwards).

!

Prototype

Prototype

Prototype

EM

QM1

QM2

FM, FS

(==QM2)

functional

+ Vibration,

Thermal

+ Thermal-

Vacuum,

EMC, Prod.

All (min level)

Models Testing Components Performance,

Beam Test

Page 181: 2004 Ams Nim Paper Draft

AMS-02/Electronics

! "#$cX

Figure 2.170: The JMDC crate during EMC testing and a typical result.

3! 7,>! 619,.*! 0/! *+01! 9)(.,11! 01! *+,! 1,-,.*0(/! (:! .(;9(/,/*1m! 96)*0.<-6)->! *+,! ;,61<),;,/*! (:!

.(1;0.!)6>!+,6D>!0(/!0/=<.,=!10/8-,!,D,/*!<91,*1!6/=!-6*.+!<91B!!J6A-,!"B$"!1<;;6)0[,1!*+,!),1<-*1!(:!*+,!

:0D,!+,6D>!0(/!*,1*!A,6;!.6;9608/1!-,=!A>!*+,!4GJ!*,6;!/,,=,=!:()!*+,!345!,-,.*)(/0.1B!!'08<),!"B$E"!

1+(?1! *+,! 1,*! <9! (:! (/,! (:! *+,! *,1*! .6;9608/1! 6/=! '08<),!"B$E%! 1+(?1! *+,! *,1*! 1,*<9! :()! *+,! d4SL!

9)(.,11()B!!!

!

Date! Location! Ions!LET

p4,Ya;8a.;"q!

Components

Tested / Pass!

F(DrOO! f5G2!S6);1*6=*! s,2!3<2!U! &!#!CX! "$!a!$$!

F(DrO$! f5G2!S6);1*6=*! e)2!3<! %!#!cO! $X!a!$\!

S,.rO$! f5G2!S6);1*6=*! U! $X!#!%O! E!a!c!

46>rO"! f5G2!S6);1*6=*! U! $&!#!CX! %%!a!"X!

',ArO%! QF52!L6*6/06! e)! "E!#!%X! &!a!C!

!

Table 2.12: Heavy ion test beam campaigns for AMS electronics component selection.

!

Page 182: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$CO!

Thermal Balance

Phase

Pump

Down

Chamber Environments: Pressure!1.0x10-5 mbar

Return

To

Ambient

Ambient

Hot

non-operation

(+85oC)

Temperature

(Proto-flight

Test Level)

Thermal Cycling Phase

Hot

Operation

(+55oC)

Cold

non-operation

(-45oC)

Cold

Operation

(-25oC)

A B C D E F G H I J K L M

2 hrsHot soak

Hot Balance

Cold

Balance

Transient

Cool-Down

1 hr

1 hr 1 hr

1

hr

1 hr

Operation (on)

Non-operation (off)

1 hr 1

hr Turn off

Turn on

2 hrsHot soak

2 hrscold soak

2 hrscold soak

N O P Q

Thermal Balance

Phase

Pump

Down

Chamber Environments: Pressure!1.0x10-5 mbar

Return

To

Ambient

Ambient

Hot

non-operation

(+85oC)

Temperature

(Proto-flight

Test Level)

Thermal Cycling Phase

Hot

Operation

(+55oC)

Cold

non-operation

(-45oC)

Cold

Operation

(-25oC)

A B C D E F G H I J K L M

2 hrsHot soak

Hot Balance

Cold

Balance

Transient

Cool-Down

1 hr

1 hr 1 hr

1

hr

1 hr

Operation (on)

Non-operation (off)

1 hr 1

hr Turn off

Turn on

2 hrsHot soak

2 hrscold soak

2 hrscold soak

N O P Q

Figure 2.171: The JMDC crate before installation in the thermal vacuum

chamber and the thermal vacuum test profile.

!

y99388Battiston !!

Figure 2.172: Radiation tests in heavy-ion beam for electronic component

selection at the INFN Catania accelerator.

Page 183: 2004 Ams Nim Paper Draft

AMS-02/Electronics

! "#$C$

Figure 2.173: JMDC under beam test at GSI.

!

46/>!(:! *+,! (*+,)! .+6--,/8,1! (:! (9,)6*0/8! 96)*0.-,! 9+>10.1! ,-,.*)(/0.1! 0/! 196.,! 6),!;,*! A>! *+,!

*+,);6-! 6/=!;,.+6/0.6-!=,108/!(:! *+,!,-,.*)(/0.1! ,/.-(1<),1!6/=! *+,);6-! .(/*)(-! 1>1*,;B! !31! 1+(?/! 0/!

'08<),!"B$Ec2!*+,!.0).<0*!A(6)=1!6),!0/*,).(//,.*,=!?0*+!A6.79-6/,1!6/=!,/.-(1,=!0/!.)6*,1!6/=!*+,!SL!*(!

SL! .(/D,)*,)1! 6),! ,/.-(1,=! 0/! A(V,1B! ! J(! .((-! *+,! ,-,.*)(/0.1! 6/=! *(!;0/0;0[,! *+,! +,6*! :-(?! 0/*(! *+,!

.)>(8,/0.1!1>1*,;2!;(1*!(:!*+,!,-,.*)(/0.1!6),!;(</*,=!(/!*+,!*?(!-6)8,!)6=06*()1!1+(?/!0/!'08<),!"B$ECB!!

31!1<;;6)0[,=!0/!J6A-,!"B$%2!345!+61!=,108/,=!6/=!A<0-*!:()!:-08+*!(D,)!&OO!1<.+!.0).<0*!A(6)=1!(:!EO!

=0::,),/*!*>9,1!?+0.+!?0--!A,!0/1*6--,=!0/!&O!.)6*,1!6/=!A(V,1!(:!6!=([,/!*>9,1B!!!

!

Figure 2.174: Electronics crates (left) and power distribution boxes (right).

CPC 700

Bridge

PPC 750

CPU

Ion Beam

Direction

Page 184: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$C"!

Figure 2.175: AMS-02 with electronics mounted on the main wake and ram radiators.

Nominal Heat (W) Weight (kg)

Crate xPD Qty Function (tot det) Boards Unit Sum extern. Subsys Unit Subsys

E-Crate 12 10.2 6.5

EHV 3*8 6.3 11.1

EPD

2 ECAL (324 PMT)

5 5.0

43.1 44.7 88

3.3

41.7

J-Crate DAQ(MDC+JxIF) 23 28.0 14.2

JT-Crate DAQ(Trig+JINJ) 8 3.8 5.6

JPD

1

J+JT power 8 18.8

50.5 50

9.2

29.1

M-Crate 12 16.5 6.8

MPD 1

Monitor, AST, GPS & Laser Align. 3 15.4

31.8 (ASTC +GPS)

46 1.9

8.7

R elec 12

RHV 2*8 7.2 6.6

RPD

2 RICH (680 PMT)

5 8.7

31.9 30.0 62

3.1

19.4

S-Crate 8 25.8 5.0

SHV 6 2.6 3.4

SPD

4 Scint(34ToF+8ACC)

3 9.4

150.8 16.8 168

1.9

41.0

T-Crate 20 37.7 11.1

TPD 8 Tracker (192 Ladder)

10 25.1 502.1 138.3 640

6.5 140.9

TT-Crate 8 17.3 4.5

TTPD 1

Tracker Thermal Elec. (1H1C) 4 15.0

32.3 (TTCB) 136 3.2

7.6

U-Crate 17 19.1 9.0

UPD 2 TRD (82 Module)

9 16.6 71.4 19.4 91

5.8 29.6

UG-Crate 12 13.2 6.5

UGPD 1 TRD Gas Elec

7 5.5 18.7 (UGB) 83

4.8 11.3

Table 2.13: Electronics weight and power.

Page 185: 2004 Ams Nim Paper Draft

AMS-02/Electronics

! "#$C%

2.8.6 Software

'08<),!"B$E&!1+(?1!*+,!.(//,.*0(/1!(:! *+,! *+),,! *>9,1!(:!9)(.,11()1!<1,=!0/!345#O"P! ! *+,!:(<)!

:(-=! ),=</=6/*!460/!S3g!L(;9<*,)1! Kd4SLN! A61,=! 6)(</=! 6! 9(?,):<-! I(?,)IL! ECO! 9)(.,11()2! *+,!

+</=),=1!(:!S080*6-!508/6-!I)(.,11()1!KS5IN!:()!1.0,/.,!=6*6!+6/=-0/8!6/=!*+,!;0.)(.(/*)(--,)1!:()!1-(?!

.(/*)(-!KU5L4NB!!3--!(:!*+,1,!9)(.,11()1!),H<0),!),-06A-,!9)(8)6;;0/8B!!G/!6==0*0(/2!*(!*,1*!6/=!=,D,-(9!

*+01!1(:*?6),!6/=!*+,!+6)=?6),!(/!?+0.+!0*!)</12!6!-6)8,!1<0*,!(:!6==0*0(/6-!1(:*?6),!01!),H<0),=B!!!

!

!!

Figure 2.176: AMS-02 processors

!

G/! ,6.+! (:! *+,! 9)(.,11()1! *+,! 1(:*?6),! 01! =0D0=,=! 0/! *?(! 96)*1B! ! 3! 10;9-,! A61,-0/,! 9)(8)6;! 01!

-(6=,=!?+,/!*+,!9)(.,11()!01!A((*,=B!!J+01!:0V,=!96)*!9)(D0=,1!;0/0;6-!:</.*0(/6-0*>!6/=!1*(),=!0/!6!(/,!

*0;,! 9)(8)6;;6A-,! ;,;()>B! ! J+,! (*+,)! 96)*! 01! *+,! ;60/! 1(:*?6),! ?0*+! :<--! :</.*0(/6-0*>B! ! G*! 01!

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!

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!!

Figure 2.177: Input and Output Rates

!!

Figure 2.178: Study of Trigger Rate and Software Parameters.

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!!

Figure 2.179: Time allotted at each step in the DAQ chain.

!

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!

!!

Figure 2.180. Flow Chart of DSP Software.

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!

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Figure 2.181: JMDC software architecture.

!

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!

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!!

Figure 2.182: Software for test and flight use.

!!

Figure 2.183: JMDC software test setup.

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!

!!

Figure 2.184: Screenshot of JPD Command & Monitor Software.

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AMS-02/Electronics

!"#$&O!

2.8.7 Electronics Process and Production!

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!

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AMS-02/Electronics

! "#$&$

!

!

!

Figure 2.185: Thermal test chamber (upper) and PCB production facilities (lower)

made available to AMS at CSIST.

Page 194: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$&"!

Figure 2.186: AMS Antimatter Investigation System (AIS).

2.8.8 Star Tracker

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!

AAS: AMS Antimatter Simulator

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AMS-02/Electronics

! "#$&%

!!

Figure 2.187: Star tracker telescopes mounted to the silicon tracker structure.

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Page 196: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$&c!

!!

Figure 2.188: Star tracker optics (a) and support (b).

!

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35GL!*(!.(/D,)*!*+,!fI5!108/6-1!6/=!,;0*!6!*0;0/8!9<-1,2!?+0.+!01!<1,=!*(!),1,*!6!-(.6-!*0;,)!?0*+0/!*+,!

*)088,)!1>1*,;B!!G/*,):6.,!,-,.*)(/0.1!?0*+0/!*+,!4#L)6*,!*+,/!),.,0D,!*+,!9),.01,!*0;,!6*!?+0.+!*+,!9<-1,!

?61!,;0**,=!6/=!*+01!01!0/.-<=,=2!6-(/8!?0*+!*+,!D6-<,!(:!*+,!-(.6-!*0;,)2!0/!*+,!,D,/*!=6*6B!!J(!),6.+!*+,!

),H<0),=! 6..<)6.>2! *+,! 1(:*?6),! )<//0/8! 0/! *+,! </0*! +61! A,,/! 19,.06-->! =,D,-(9,=! *(! 0/.-<=,! 6--! *+,!

.()),.*0(/1!),H<0),=!?+,/!*)6D,-0/8!0/!-(?!,6)*+!()A0*B!!!

!

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AMS-02/Electronics

! "#$&C

!!

Figure 2.189: TOPSTAR 3000D unit and a GPS patch antenna.

!

2.8.10 AMS Ground Data Handling and Remote Commanding!

J+,! -(/8! =<)6*0(/! (:! 345#O"! ;0110(/! (/! *+,! G/*,)/6*0(/6-! 596.,! 5*6*0(/! KG55N! ;67,1! *+,!

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J+,1,!.(;9<*,)1!?0--!+6D,!*(!)</!</6**,/=,=!"c!+(<)1!9,)!=6>2!E!=6>1!9,)!?,,72!*+<1!1>1*,;!),-06A0-0*>!01!

*+,!D0*6-!011<,B!!J+,!1>1*,;!1+(<-=!A,!6A-,!*(!1*(),!6A(<*!"!?,,71!(:!=6*6B!!J?(!0=,/*0.6-!1>1*,;1!?0--!A,!

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196.,! 1*6*0(/2! *+,! IMLL! ?0--! A,! -(.6*,=! 6*! L@RF2! ?0*+! 6! A6.7<9! -(.6*0(/! 6*! 4GJB! @V*,/10D,! =6*6!

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=0::,),/*!8,(8)69+0.6-!-(.6*0(/1!6*!*+,0)!+(;,!0/1*0*<*,1B!

Page 198: 2004 Ams Nim Paper Draft

AMS-02/Electronics

!"#$&&!

!

!

!

Fig

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0: D

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Page 199: 2004 Ams Nim Paper Draft

AMS-02/Electronics

! "#$&E

J+,!5ML2!61!1+(?/!0/!'08<),!"B$X$2!),.,0D,1!6/=!1*(),1!6--!345!1.0,/.,!6/=!+(<1,7,,90/8!=6*62!

61!?,--!61!6/.0--6)>!=6*6!:)(;!F3532!,/1<),1!:<--!1.0,/.,!=6*6!),.(/1*)<.*0(/2!.6-0A)6*0(/!6/=!6-08/;,/*!

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),H<0),=! *(! ),.(/1*)<.*!345#O"! 1.0,/.,! =6*62! .6-0A)6*,! 6/=! 6-08/! *+,! =,*,.*()1! 6/=! 1*(),! *+,! ),1<-*1! (:!

),.(/1*)<.*0(/!61!?,--!61!4(/*,!L6)-(!10;<-6*0(/1B!!3!5ML!9)(*(*>9,!+61!A,,/!1,*<9!6*!L@RF!6/=!01!0/!

<1,! :()! 345#O"!4(/*,! L6)-(! 10;<-6*0(/B! ! J+,! 5ML! ,D,/*! ),.(/1*)<.*0(/! :6.0-0*>! ?0--! ,/1<),! *+,! :<--!

),.(/1*)<.*0(/!(:!6A(<*!$O`!(:!*+,!0/9<*!,D,/*1!?0*+!6/!6D,)68,!*0;,!=,-6>!(:!/(!;(),!*+6/!+6-:!6/!+(<)!

6/=!,/1<),!*+,!:<--!),.(/1*)<.*0(/!(:!$OO`!(:!*+,!,D,/*1!?0*+!6!*>90.6-!=,-6>!*0;,!(:!-,11!*+6/!(/,!=6>B!!!

J+,!.(;9-,*,!f)(</=!S6*6!T6/=-0/8!6/=!R,;(*,!L(;;6/=0/8!5>1*,;!01!1.+,=<-,=!*(!A,!<9!6/=!

)<//0/8! 10V!;(/*+1! A,:(),! 345! -6</.+! *(! 1<99()*! 345! *,1*0/8! 6*! e5L! 6/=! *+,! ,6)->! 0/1*6--6*0(/! (:!

3LMI!(/!*+,!G55B!!!

!

!!

Figure 2.191: The AMS Science Operations Center (SOC) at CERN.

Page 200: 2004 Ams Nim Paper Draft

AMS-02/Thermal

!"#$%&!

2.9 Thermal Control

'()! *()+,-.! )/01+2/,)/*! 1/! 34-5)! 13! (-+3(6! ! 7188)+)/*! -+)-3! 28! *()! 9)*)5*2+! -+)! 3:;<)5*)9! *2!

+-419.=!0-+=1/>!91+)5*!32.-+!1..:,1/-*12/!-.*)+/-*1/>!?1*(!)@423:+)!*2!9))4!34-5)A!9)4)/91/>!2/!*()!2+;1*-.!

4-+-,)*)+3!28! *()!34-5)!3*-*12/6! !'?2!B1.2?-**3!28!42?)+! 13!913314-*)9!?1*(1/! *()!)@4)+1,)/*6! !C-+=1/>!

+-91-*12/! 8+2,!D-+*(!,:3*!-.32!;)! *-B)/! 1/*2!-552:/*6! !'()! *()+,2#24*15-.!4+24)+*1)3!28! *()!)@4)+1,)/*!

5(-/>)!?1*(! *1,)6! ! E/! *(13! )/01+2/,)/*A! ;)5-:3)! *()! +)342/3)! 28! *()! 9188)+)/*! 9)*)5*2+3! 13! *),4)+-*:+)!

9)4)/9)/*A!*()1+!*),4)+-*:+)!,:3*!;)!B)4*!/2*!2/.=!?1*(1/!*()1+!9188)+)/*!24)+-*12/-.!+-/>)3!;:*!1*!,:3*!;)!

B)4*! 3*-;.)! 20)+! ;2*(! *1,)! -/9! 02.:,)6! ! F23*! 5+1*15-..=A! *()! 42331;1.1*=! 28! -/=! ()-*! .)-B1/>! 1/*2! *()!

3:4)+8.:19!().1:,!3:44.=A!?(15(!9)*)+,1/)3! *()!9:+-*12/!28! *()!)@4)+1,)/*! 82+!,-/=!4(=3153! 5(-//).3A!

,:3*! ;)! ,1/1,1G)96! ! H2+! *()3)! +)-32/3A! *()! '()+,-.! I2/*+2.! J=3*),! K'IJL! 82+! MFJ#N"! (-3! ;))/!

9)31>/)9!-/9!13!:/9)+!52/3*+:5*12/!-/9!*)3*1/>!;=!D'O!PQ+15(A!FE'A!RJST!-/9!J(-/92/>!U/10)+31*=!1/!

52..-;2+-*12/!?1*(!*()+,-.!52/*+-5*2+3!I-+.2!V-0-GG1!J4-5)!-/9!TOW!J=3*),6!!D@*)/310)!,29).1/>!-/9!

*)3*1/>! (-3! ;))/! 4)+82+,)9! -/9! *()! *()+,-.! 52/*+2.! 3=3*),! ?1..! ;)! 0-.19-*)9! 1/! -/! 20)+-..! '()+,-.!

C-5::,!')3*!28!*()!52,4.)*)!)@4)+1,)/*!3:442+*)9!;=!*()!D:+24)-/!J4-5)!M>)/5=!KDJML6!

2.9.1 Thermal environment

'()! 4+1,-+=! )@*)+/-.! 8-5*2+! 1/! *()! *()+,-.! )/01+2/,)/*! 13! 32.-+! 1..:,1/-*12/6! ! '(13! 9)4)/93!

4+1,-+1.=!2/! *()!-/>.)!;)*?))/! *()!EJJ!2+;1*-.!4.-/)!-/9! *()!91+)5*12/! *2! *()!J:/6! !'()!X;)*-Y!-/>.)! 13!

1..:3*+-*)9!1/!H1>:+)!"6$Z"-6!!H2+!*()!EJJ!2+;1*-.!1/5.1/-*12/!K[$6%\L!-/9!*()!*1.*!28!*()!D-+*(]3!-@13!K"^6[\LA!

*()!;)*-!-/>.)!0-+1)3!;)*?))/!!_[6$\!-/9!`_[6$\A!,29:.-*)9!;=!*()!3)-32/3!-3!3(2?/!1/!H1>:+)!"6$Z";6!!

H2+!;)*-!-/>.)3!?1*(!,->/1*:9)3!>+)-*)+! *(-/!_N\! *()!2+;1*! 13!)/*1+).=! 1/!3:/.1>(*A!?(1.)! 82+!;)*-!-/>.)3!

/)-+!N\!-;2:*!aNb!28!*()!2+;1*!13!1/!*()!D-+*(]3!3(-92?!KH1>:+)!"6$Z^-L6!!H2+!*()!,-<2+1*=!28!*()!*1,)A!*()!

;)*-! -/>.)! .1)3! ?1*(1/! ![N\! *2! `[N\! KH1>:+)!"6$Z^;L6! ! '()! 1/*)/31*=! 28! *()! 32.-+! 1..:,1/-*12/A! 2+! 32.-+!

52/3*-/*A!-.32!0-+1)3!-//:-..=!?1*(!*()!913*-/5)!*2!*()!3:/A!8+2,!$^""!*2!$a"a!cd,"!-*!5.23)3*!-44+2-5(!

KH1>:+)!"6$Za-L6!!!

!

-100.0

-75.0

-50.0

-25.0

0.0

25.0

50.0

75.0

100.0

0 500 1000 1500 2000

Time (days)

Be

ta a

ng

le (

de

gre

es)

!!

Figure 2.192: Beta angle definition (a) and variation (b).

!

7188)+)/*! 4-+*3! 28! MFJ! -+)! )@423)9! *2! 9188)+)/*! -,2:/*! 28! 91+)5*! 3:/.1>(*! -*! 9188)+)/*! *1,)3A!

9)4)/91/>!2/!*()!EJJ!-**1*:9)A!?(15(!13!)@4+)33)9!1/!*()!-)+2/-:*15-.!522+91/-*)3!28!=-?A!41*5(!-/9!+2..6!!

'()3)!-+)!)@4)5*)9!*2!0-+=!;=!:4!*2!e"N\6!!!I2,4.15-*1/>!*(13!13!*()!3(-92?1/>A!1/!32,)!-**1*:9)3A!28!4-+*3!

28!*()!)@4)+1,)/*!;=!9188)+)/*!4-+*3!28!*()!34-5)!3*-*12/!-/9!*()!+-91-*12/!+)8.)5*)9!2/*2!9188)+)/*!4-+*3!28!

*()!)@4)+1,)/*!;=!9188)+)/*!34-5)!3*-*12/!).),)/*36!!'()!EJJ!-.*1*:9)!5-/!-.32!0-+=!8+2,!"__!*2![NN!B,6!

(a) (b)

Page 201: 2004 Ams Nim Paper Draft

AMS-02/Thermal

! "#$%Z

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

0 10 20 30 40 50 60 70 80

beta (degrees)

Fra

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it i

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5-3)3!?1*(1/!e![N\

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.%/+'0+1"%'2*%3&%%-4

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!!

Figure 2.193: Fraction of orbit in sunlight vs. beta angle (a). Number of days per beta angle (b).

!

! O)-*! 8+2,! *()!D-+*(! 13!-552:/*)9! 82+! 1/! *?2!?-=36! !'()! *),4)+-*:+)!28! *()!D-+*(! -3! 3))/! 8+2,!

34-5)!0-+1)3!8+2,!"a[!*2!"%%!f!KH1>:+)!"6$Za;L6!!'()!-.;)92!52/3*-/*A!?(15(!13!-33251-*)9!?1*(!+)8.)5*)9!

32.-+!+-91-*12/!-.32!0-+1)3!8+2,!"N!*2!aNb!KH1>:+)!"6$Za5L6!!!

! E/! -991*12/A! *()! *()+,2#24*15-.! 4+24)+*1)3! K),133101*=! -/9! -;32+4*101*=L! 28! *()! )@423)9!

)@4)+1,)/*-.! 3:+8-5)3! 5(-/>)! ?1*(! *1,)6! ! '()! )02.:*12/! 28! -! *=415-.! ,-*)+1-.! 4+24)+*=! 13! 3(2?/! 1/!

H1>:+)!"6$Za96!!!

!

Solar Constant

1260

1280

1300

1320

1340

1360

1380

1400

1420

1

92

18

3

274

365

456

547

63

8

729

820

911

10

02

1093

Time (days)

W/m

^2

EARTH TEMPERATURE

230

235

240

245

250

255

260

265

270

1 201 401 601 801 1001 1201 1401 1601 1801

Days

Te

mp

era

ture

(K

)

Albedo

05

1015202530354045

1 201 401 601 801 1001 1201 1401 1601

Days

Alb

edo

(%

)

BOL-EOL t/o properties

0.1

0.12

0.14

0.16

0.18

0.2

0.22

0.24

1 201 401 601 801 1001

Days

Wh

ite

pa

int a

bsorp

tivity

!!

Figure 2.194: Factors effecting external thermal environment: Solar constant (a),

Earth temperature (b), Albedo (c), Beginning of life (BOL) to End of

life (EOL) properties of white paint (d) [1].

!

(a)

(d)

(b)

(a) (b)

(c)

Page 202: 2004 Ams Nim Paper Draft

AMS-02/Thermal

!"#$_N!

E/*)+/-..=!*2!*()!)@4)+1,)/*A!*()!*()+,-.!)/01+2/,)/*!13!-.32!52,4.)@A!-3!3(2?/!1/!H1>:+)!"6$Z[6!!

'()!,->/)*!-/9!3:++2:/91/>!*-/B!28!3:4)+8.:19!().1:,!-+)!-*!$6&!f6!!M*!*()!0-42+!522.)9!3(1).9!5.23)3*!*2!

*()!2:*319)!28!*()!*2+219-.!0-5::,!5-3)!KCIJaA!H1>:+)!"6[L!*(13!(-3!+13)/!*2!-;2:*!%&!fA!,-1/*-1/)9!;=!*()!

82:+!5+=2522.)+3!?(15(!,:3*! +-91-*)!aNN!c!28! 1/4:*!42?)+!4.:3! *()!:4! *2!^"!c!28!()-*! .18*)9! 8+2,!*()!

5+=2>)/153! 3=3*),6! ! '()! 0-5::,! 5-3)! *),4)+-*:+)! 0-+1)3! -+2:/9! "_N!f6! ! '()! *+-5B)+! 31*3! ?1*(1/! *()!

0-5::,!5-3)! -//:.:3! -/9!913314-*)3!$aa!c6! !M;20)! *(13! -+)! *()!U44)+!'TH!-/9!'g7A!?(15(! *2>)*()+!

913314-*)! "^!c6! ! W).2?! -+)! *()! h2?)+! 'TH! Ka!cLA! gEIO! K^_!cL! -/9! *()! DIMh! K_"!cL6! ! M..! 28! *()!

9)*)5*2+3!,:3*! 24)+-*)! -*! 2+! /)-+! N!,I6! !'()! ).)5*+2/153A!?(15(!,:3*! ;)! .25-*)9! 5.23)! *2! *()! 9)*)5*2+3A!913314-*)!*()!;-.-/5)!28!*()!1/4:*!42?)+!Ki$[NN!cL!*(2:>(!1*!92)3!(-0)!-!?19)+!24)+-*12/-.!*),4)+-*:+)!

+-/>)6!!M..!28!*()3)!).),)/*3!-+)!*()+,-..=!1/*)+52//)5*)9!;=!+-91-*12/!-/9!52/9:5*12/!*(+2:>(!52,,2/!

3:442+*!3*+:5*:+)3!-/9!5-;.1/>6!!!

!

!!

Figure 2.195: Thermal dissipation of AMS-02 detectors

!!!!!KFhE!13!,:.*1#.-=)+!1/3:.-*12/L6!

!

!

!

!

TRD (20 W): Indirect radiation,

Enclosed in MLI Upper TOF (3 W): Enclosed in MLI

with TRD ACC (1 W): Direct Radiation Tracker (144 W): Dedicated

pumped two phase loop. Magnet+Cryocoolers (4x108 W):

Capillary pumped loops to Zenith Rad.

Lower ToF (4 W): Direct Radiation

RICH (37 W): Direct Radiation ECAL (72 W): Direct Radiation

+ Conduction to USS.

Page 203: 2004 Ams Nim Paper Draft

AMS-02/Thermal

! "#$_$

2.9.2 Thermal requirements

D-5(!28!*()!9)*)5*2+!).),)/*3!(-3!34)51815!*()+,-.!+)j:1+),)/*36!!'()!?19)3*!.1,1*3!-+)!*()!/2/#

24)+-*12/-.A!2+!3*2+->)A!.1,1*36!!E8!*()!*),4)+-*:+)!28!*()!).),)/*3!13!-..2?)9!*2!)@5))9!*()3)!.1,1*3A!*()=!

,-=!;)!9-,->)96! !c1*(1/! *()3)! .1,1*3!-+)! *()!24)+-*12/-.! .1,1*3! *(-*!,:3*!;)!,-1/*-1/)9!82+! *()!4+24)+!

8:/5*12/!28!*()!1/3*+:,)/*36!!'()3)!-+)!9)81/)9!1/!*)+,3!28!*()!-;32.:*)!*),4)+-*:+)!+-/>)A!1/!*)+,3!28!*()!

*),4)+-*:+)! 0-+1-*12/! K.'L! 20)+! *1,)! -/9! 1/! *)+,3! 28! *()! 0-+1-*12/! 20)+! *()! 02.:,)! 28! *()! ).),)/*6!!'-;.)!"6$^!3:,,-+1G)3!*()3)!.1,1*3!82+!*()!,-<2+!).),)/*36!!E/!-991*12/A!*()!*),4)+-*:+)3!28!*()!'g7!>-3!

*-/B3!(-0)!*2!;)!B)4*!-;20)!$_!,I!82+!k)!-/9!^$!,I!82+!IT"!*2!;)!-;.)!*2!9)*)+,1/)!*()!-,2:/*!28!>-3!+),-1/1/>!;=!,)-3:+1/>!*()!4+)33:+)6!!T*()+!).),)/*3!KIMWA!''IWA!)*5L!(-0)!*()1+!2?/!+-/>)36!!!

!

Element Dissipation

[W]

Non-

Operational Operational

Max .T

per orbit

Max .T over

detector volume

'g7! "N! l!"NA!`aNm! l`$NA!`"[m! "! $!

'+-5B)+!K31.152/L! N! l!"NA!`aNm! l!$NA!`"[m!

'+-5B)+!K(=;+19L! $aa! l!"NA!`%Nm! l!$NA!`aNm!

^!

K$Nd9-=L!$N!

C-5::,!I-3)! ! $!`$N! ! !

I+=2522.)+3! a^"! l!$NA!`aNm! l!$NA!`"Nm! ! !

gEIO! ^_! l!^[A!`%Nm! l!^NA!`[Nm! _! $[!K-,2/>!SF'3L!

DIMh! _"! l!aNA!`aNm! l!"NA!`aNm! [! $N!KSF'!*2!3*+:5*:+)L!

'TH! ^`a! l!aNA!`%Nm! l!^NA!`[[m! [! $N!KSF'!*2!3*+:5*:+)L!

MII! $! l!"NA!`aNm! l!"NA!`aNm! ! !

D.)5*+2/153! $[NN! l!^NA!`[[m! l!"NA!`[Nm! ! !

!

Table 2.14: Summary of thermal requirements of major AMS-02 elements, in degrees Celsius.

!

E/!-991*12/!*2!*()3)!+)j:1+),)/*3A!*()!()-*!8.2?!1/*2!*()!5+=2,->/)*!,:3*!;)!,1/1,1G)9A!32!()-*!

8+2,!/)-+;=! 32:+5)3!,:3*! ;)! B)4*! -?-=6! ! E/! 4-+*15:.-+A! *()! *+-5B)+! 913314-*12/! 1/319)! *()! 0-5::,! 5-3)!

-//:.:3!,:3*!;)!52..)5*)9A!52/9:5*)9!2:*319)!*()!0-5::,!5-3)!-/9!+-91-*)96!!h1B)?13)!*()!913314-*12/!28!

*()! 82:+! 5+=2522.)+3A!?(15(! -+)!,2:/*)9!2/! *()! 0-5::,!5-3)A!,:3*! ;)! 52..)5*)9! -/9! *+-/38)++)9! -?-=6!!

g-91-*10)! ()-*! .)-B3! 8+2,! *()! 2*()+! 3=3*),3! ,:3*! ;)! ;.25B)9! ?1*(! ,:.*1#.-=)+! 1/3:.-*12/! KFhEL! -/9!

52/9:5*10)!.)-B3!?1*(!1/3:.-*1/>!<21/*36!!!

W)=2/9!*()3)!+)j:1+),)/*3!-+)!9)31>/!>2-.3A!?(15(!24*1,1G)!*()!4)+82+,-/5)!28!*()!9)*)5*2+3!-/9!

*()!)/9:+-/5)!28!*()!3:4)+8.:19!().1:,6!!M3!*()!+)342/3)!28!-..!9)*)5*2+3!9)4)/9!2/!*),4)+-*:+)A!1/5+)-3)9!

3*-;1.1*=!20)+!*1,)!-/9!02.:,)!5-/!,1/1,1G)!*()!42331;1.1*=!28!3=3*),-*15!3(18*3! 1/! *()!4(=3153!-/-.=3136!!

'()!*+-5B)+!24)+-*)3!?1*(!.)33!/213)!-*!.2?)+!*),4)+-*:+)36!!'()!).)5*+2/153!+).1-;1.1*=!13!1/5+)-3)9!18!1*!13!

24)+-*1/>!-*!.2?)+!*),4)+-*:+)3A!*(2:>(!1*!13!9)31>/)9!*2!?2+B!-*!*()!,-@1,:,!*),4)+-*:+)!82+!*()!)/*1+)!

,13312/6!!'()!4)+82+,-/5)!28!*()!5+=2522.)+3!13!-!52,4.15-*)9!8:/5*12/!28!*()!*),4)+-*:+)!-*!*()!1/*)+8-5)!

28! *()1+! 52.9! *14! ?1*(! *()! 0-42+! 522.)9! 3(1).9A! *()! ;29=! *),4)+-*:+)! -/9! *()! 1/4:*! 42?)+6! ! T4*1,:,!

4)+82+,-/5)! 13! 2;*-1/)9!?()/! *()! ;29=! 28! *()! 5+=2522.)+3! 13!,-1/*-1/)9! -*! N!,I6! ! '()! *1,)! -0)+->)9!*),4)+-*:+)!28!*()!0-5::,!5-3)!,:3*!-.32!;)!B)4*!-3!.2?!-3!42331;.)6!!!

M991*12/-.!+)j:1+),)/*3!-+)!1,423)9!;=!RMJM!*2!24)+-*)!2/!*()!34-5)!3*-*12/6!!O)-*!5-/!/2*!;)!

+)<)5*)9!*2?-+93!*()!3*-*12/!).),)/*3!;).2?!MFJ!/2+!*2!*()!42+*!-/9!3*-+;2-+9!319)3!28!*()!)@4)+1,)/*6!!

O1>(.=!34)5:.-+!3:+8-5)3A!?(15(!(-0)!)@*+),).=!.2?!-;32+4*12/A!5-//2*!;)!:3)9!-3! *()=!,-=!9-GG.)! *()!

-3*+2/-:*3!2+!24*15-.!1/3*+:,)/*-*12/6!!'()!-**1*:9)!28!*()!3*-*12/A!-/9!52/3)j:)/*.=!MFJA!13!9)*)+,1/)9!

;=!2*()+! 52/5)+/3! *(-/! *()!MFJ! *()+,-.! )/01+2/,)/*A! 1/! 4-+*15:.-+! *()! /))93! *2! B))4! *()! 32.-+! -++-=3!

,-@1,-..=!1..:,1/-*)9!-/9!*2!,1/1,1G)!*()!4+24:.312/!+)j:1+)96!!

Page 204: 2004 Ams Nim Paper Draft

AMS-02/Thermal

!"#$_"!

2.9.3 Thermal design

W)5-:3)!28!*()1+!9188)+1/>!*()+,-.!+)j:1+),)/*3A!*()!20)+-..!*()+,-.!9)31>/!-44+2-5(!(-3!;))/!*2!

*()+,-..=! 3)4-+-*)A! -3! ,:5(! -3! 42331;.)A! *()3)! 9188)+)/*! ).),)/*3! -/9! -++10)! -*! -! 32.:*12/! 82+! )-5(!

1/91019:-..=6! !'()!*()+,-.!52/*+2.!3=3*),!82+!*()!*+-5B)+!?-3!9)35+1;)9!1/!n!"6^6[!-/9!82+!*()!52,;1/)9!

'g7!4.:3!U44)+!'TH!).),)/*! 1/!n!"6"6a6! !'()!3,-..!-,2:/*3!28!()-*! 8+2,!*()!h2?)+!'THA!gEIO!-/9!

DIMh!-+)! +)<)5*)9!:31/>! 3,-..! +-91-*10)! 3:+8-5)3! -**-5()9!91+)5*.=! *2! *()3)! 9)*)5*2+36! !'()!DIMh!-.32!

:3)3!*()!:/1j:)!3:442+*!3*+:5*:+)!KUJJL!;)-,3!*2!?(15(!1*!13!-**-5()9!-3!-!()-*!31/B6!!O)-0=!:3)!13!,-9)!

28!1/3:.-*1/>!3(1,3!;)*?))/!3*+:5*:+-.!,),;)+3!-/9!FhE!;)*?))/!9188)+)/*!02.:,)3!*2!,-1/*-1/!*()+,-.!

3)4-+-*12/!-/9!*2!-0219!:/52/*+2..)9!()-*!8.2?!;-5B!1/*2!*()!,->/)*6!!H2+!)@-,4.)A!;)*?))/!*()!'g7!4.:3!

U44)+!'TH!-/9! *()!0-5::,!5-3)!-!"N#.-=)+!FhE!;.-/B)*!B))43! *()! +-91-*12/! .2-9!2/! *()!0-5::,!5-3)!

;).2?! ^!c6! '()! 0-5::,! 5-3)! *),4)+-*:+)! 13! 52/*+2..)9! 4-3310).=! ;=! 3:+8-5)! *+)-*,)/*! *2! -5(1)0)! *()!

+)j:1+)9! *()+,2#24*15-.! 4+24)+*1)36! ! E/! -991*12/! *2! *()! *+-5B)+! 3=3*),A! *()! *()+,-.! 3=3*),3! 82+! *()!

5+=2522.)+3!-/9!82+!*()!).)5*+2/153!(-0)!+)j:1+)9!*()!,23*!3*:9=!*2!,))*!*()1+!+)j:1+),)/*36!!!H1>:+)!"6$Z%!

3(2?3!*()!+-91-*2+3!+)j:1+)9!82+!*()3)!*(+))!3=3*),36!!!

!

TrackerRadiator ~70 W

TrackerRadiator~70 W

WAKERadiator~750 W

RAMRadiator~750 W

Electronics - direct mounting on!

!

Figure 2.196: AMS-02 Radiators and loads (left).

Detail of Zenith ! panel and attached cooling loops (right).

!

'()! 32.:*12/! 82+! *()! 5+=2522.)+3! 13! *2! :3)! 5-41..-+=! 4:,4)9! .2243! *2!,20)! *()! ()-*! :4! *2! *()!

G)/1*(!+-91-*2+6!!D-5(!28!*()!82:+!5+=2522.)+3!13!-/!1/9)4)/9)/*A!+)9:/9-/*!3=3*),A!?1*(!*?2!)0-42+-*2+3!

,2:/*)9!2/!*()!;29=!28!*()!5+=2522.)+6!!M3!3(2?/!1/!H1>:+)!"6$Z%A!)-5(!)0-42+-*2+!8))93!-!.224!()-*!414)!

KhOSL!-/9!*()!?2+B1/>!8.:19A!-,,2/1-A!5-++1)3!*()!()-*!:4!*2!*()!G)/1*(!+-91-*2+6!!'()!*?2!.2243!8+2,!-!

5+=2522.)+!-+)!;+-G)9! *2!-!9)915-*)9!j:-+*)+!4-/).! K$!,"L!28! *()!G)/1*(! +-91-*2+A! 8+2,!?()+)! *()!()-*! 13!

+)<)5*)9! -/9! *()! 8.:19! 52/9)/3)9! -/9! +)51+5:.-*)9!;=! 5-41..-+=! 4+)33:+)6! !W)5-:3)! *()! 4-/).3! -+)! 1/! *()!

-4)+*:+)!28!*()!9)*)5*2+A!*()=!(-0)!;))/!,-9)!-3!*(1/!-/9!:/182+,!-3!42331;.)!K-!3-/9?15(!28!$6%!,,!M.A!

$N!,,!28!g2(-5).!-/9!N6^!,,!M.L!-3!(-0)!*()!52/9)/31/>!.2243!).),)/*3!),;)99)9!?1*(!*(),!KM.!*:;)3!

28!^!,,!2:*)+!91-,)*)+!?1*(!N6[!,,!?-..3L6!!'()!4-/).3!-+)!,2:/*)9!2/!81;)+!>.-33!3*-/92883!*2!1/3:.-*)!

*(),!8+2,!*()!'g76!!h1B)?13)!*()!.)-B!8+2,!5+=2522.)+3!*2!0-5::,!5-3)!13!,-1/*-1/)9!-*!.)33!*(-/![!c!

)-5(6!!!

! M3!*()!).)5*+2/153!(-0)!-!?19)!24)+-*1/>!+-/>)!-/9!92!/2*!(-0)!3*+2/>!3*-;1.1*=!+)j:1+),)/*3A!*()!

9)31>/! 28! *()! *()+,-.! 52/*+2.! 3=3*),! 13! 31,4.181)96! ! T/! *()! 2*()+! (-/9A! -.*2>)*()+! *()! 913314-*12/! 13!

i$[NN!cA! -! 31>/1815-/*! ()-*! .2-9! *(-*! ,:3*! ;)! 91+)5*)9! -?-=! 8+2,! *()! 2*()+! 9)*)5*2+! ).),)/*36! ! '()!

).)5*+2/153! 13! 52/*-1/)9! 1/! *()! ;2@)3! 3(2?/! H1>:+)!"6$Z_! .25-*)9! 2/! *()! ?-B)! -/9! +-,! 319)3! 28! *()!

Evaporators

LHP

Panel

Page 205: 2004 Ams Nim Paper Draft

AMS-02/Thermal

! "#$_^

9)*)5*2+6!!T/!)-5(!319)!*()!;2@)3!-+)!,)5(-/15-..=!.1/B)9!*2!82+,!-!3).8!3:442+*1/>!3*+:5*:+)!?(15(!34-/3!

*()! -+)-! ;)*?))/! *()! 82:+! :44)+!UJJ! ;)-,3! K3))! -.32! H1>:+)!"6$L6! ! '()! X,-1/Y! +-91-*2+3! -+)!,2:/*)9!

91+)5*.=!*2!*()!;2@)36! !O)-*!8+2,!*()!).)5*+15-.!52,42/)/*3!13!52/9:5*)9!8+2,!*()!4+1/*)9!51+5:1*!;2-+93!

KSIW3L!*2!*()!;2@!?-..3!2+! *2!8+-,)3!?(15(!(2.9!*()!;2-+936! !E*! 13! *()/!52/9:5*)9!91+)5*.=!*2!*()!1/319)!

3:+8-5)! 28! *()! -**-5()9! +-91-*2+3A!?(15(! -+)! -.32!,-9)! 28! -/!M.og2(-5).oM.! 3-/9?15(6! !M,,2/1-! ()-*!

414)3! ?1*(1/! *()! +-91-*2+3! )/3:+)! *()! *+-/38)+! 28! *()! ()-*! 8+2,! *()! 1/319)! *2! *()! 2:*319)! -/9! -.32! *()!

913*+1;:*12/! 28! *()! ()-*! )0)/.=! 20)+! *()! )/*1+)! -+)-! Ka!,"L! 28! *()! +-91-*2+6! !g-91-*12/! ;-5B! *2?-+93! *()!

9)*)5*2+3!-/9!0-5::,!5-3)!13!;.25B)9!Kp^bL!;=!3:+8-5)!*+)-*,)/*!28!*()!1//)+!+-91-*2+!3:+8-5)3!-/9!FhE!

-+2:/9!*()!;2@)36!!!

!

!!

Figure 2.197: Main ram (right) and wake (left) radiators mounted on the structure of linked

electronic boxes K+-,!+)8)+3!*2!*()!EJJ!91+)5*12/!28!*+-0).A!?-B)!13!244231*)L6!!

!

2.9.4 Thermal integration and modeling

F29).1/>!28! *()! *()+,-.!4)+82+,-/5)!28!MFJ!(-3!;))/!-!,:.*1#3*)4A! 1*)+-*10)!4+25)9:+)6! !H1+3*!

*()!)@4)+1,)/*!?-3!34.1*!1/*2!*()!9188)+1/>!*()+,-.!).),)/*3!9)35+1;)9!-;20)!-/9!1/*)+8-5)3!;)*?))/!*()3)!

).),)/*3! ?)+)! 9)81/)96! ! 7)*-1.)9! ,29).1/>! 13! 92/)! 82+! )-5(! ).),)/*! ;-3)9! 2/! ;2:/9-+=! 52/91*12/3!

3:44.1)9!8+2,!*()!20)+-..!*()+,-.!,29).6!!g)3:.*3!8+2,!*()!9)*-1.)9!,29).1/>!-+)!*()/!1/5.:9)9!;-5B!1/*2!

*()!20)+-..!,29).!1/!*)+,3!28!()-*!8.2?!-5+233!*()!1/*)+8-5)3A!*()!20)+-..!,29).!13!+)-/-.=G)9!-/9!+)3:.*3!

3:44.1)9!->-1/!*2!*()!9)*-1.)9!,29).36!!W=!9)31>/A!*()!).),)/*3!-+)!-3!*()+,-..=!1/9)4)/9)/*!-3!42331;.)A!

32! *(13! 4+25)9:+)! 52/0)+>)3! -8*)+! <:3*! -! 8)?! 1*)+-*12/36! ! W-3)9! 2/! *()! +)3:.*3A! *()! *()+,-.! 9)31>/3! -+)!

-9<:3*)9!-/9!*()!4+25)9:+)!+)3*-+*)9!:/*1.!-..!*()!+)j:1+),)/*3!-+)!,)*!-/9!*()!9)31>/!>2-.3!-44+2-5()96!!!

M..! 28! *(13! ,29).1/>! ,:3*! ;)! 92/)! 1/! *()! 0-+=1/>! )@*)+/-.! *()+,-.! )/01+2/,)/*6! ! '()! ,-1/!

)/01+2/,)/*-.!8-5*2+3A!;)*-!-/>.)!-/9!EJJ!-**1*:9)!-+)!;1//)9!1/*2!$&Z!5-3)36!!H2+!)-5(!).),)/*A!*()!?2+3*!

(2*!5-3)A! *()!?2+3*!52.9!5-3)!-/9A! 18! +)j:1+)9A! *()!?2+3*!34-*1-.!0-+1-*12/!5-3)A!-+)! 19)/*181)9! 8+2,!*()3)!

$&Z!5-3)3!:31/>! *()!-44+24+1-*)!?2+3*! EJJ!-.*1*:9)A! 32.-+!52/3*-/*A!D-+*(! *),4)+-*:+)A!-.;)92!-/9!WTh#

DTh!4+24)+*1)36! ! E/!-991*12/A! *()!24)+-*1/>! +-/>)!,:3*!;)!,)*!?()/! *()!).),)/*! 13!913314-*1/>!-/9! *()!

Page 206: 2004 Ams Nim Paper Draft

AMS-02/Thermal

!"#$_a!

/2/#24)+-*1/>! +-/>)!,)*!?()/! 1*! 13! /2*6! ! '()! )02.:*12/! 28! *),4)+-*:+)3! 13! 3*:91)9! 20)+! *1,)! :31/>! $"!

3)j:)/*1-.! 4231*12/3! 20)+! )-5(! 2+;1*6! ! '()3)! 91,)/312/1/>! 5-3)3! 9+10)! *()! *()+,-.! 9)31>/! ?(15(! ,:3*!

;-.-/5)!*()!522.1/>!+)j:1+)9!1/!*()!?2+3*!(2*!24)+-*1/>!5-3)!?1*(!*()!()-*1/>!+)j:1+)9!1/!*()!?2+3*!52.9!

/2/#24)+-*1/>! 5-3)6! !T?1/>! *2! *()! 9188)+)/*! +)j:1+),)/*3! 28! *()! 9)*)5*2+! ).),)/*3! -/9! *2! *()! 9188)+)/*!

)/01+2/,)/*-.!8-5*2+3!*2!?(15(!*()=!-+)!)@423)9A!*()!91,)/312/1/>!5-3)3!-+)!9188)+)/*!82+!)-5(!).),)/*6!!

'=415-..=A!*()=!255:+!-*!52,;1/-*12/3!28!-/!)@*+),)!;)*-!-/>.)!-/9!-/!)@*+),)!=-?!2+!+2..!-/>.)6!!!

'(2:>(!28!3(2+*)+!9:+-*12/A!*()!*()+,-.!)/01+2/,)/*3!-/9!*()+,-.!+)342/3)!?()/!MFJ!13!1/!*()!

34-5)!3(:**.)!4-=.2-9!;-=!-/9!?()/!1*!13!;)1/>!*+-/38)++)9!8+2,!*()!34-5)!3(:**.)!*2!*()!34-5)!3*-*12/!(-0)!

-.32! ;))/! )@-,1/)96! ! H2+! 32,)! ).),)/*3A! *()! *+-/38)+! 4(-3)! (-9! ;)52,)! *()! 91,)/312/1/>! 52.9! /2/#

24)+-*12/! 5-3)6! ! '2! -0219! *(13A! *()! ).)5*+15-.! 9)31>/! 28! *()!S7J! KH1>:+)!"6$[&L!?-3!,29181)9! *2! -55)4*!

42?)+!8+2,!*()!34-5)!3*-*12/!-+,!*2!3:44.=!()-*)+36!!!

')5(/15-..=A!*()!,29).1/>!13!92/)!;=!,-/=!9188)+)/*!52..-;2+-*2+3!:31/>!*()!328*?-+)!,23*!3:1*)9!

*2!*()1+!/))93!KDJM'MRA!JER7MdHhUER'A!E7DMJ#'FVA!-9!(25!H2+*+-/!529)3A!'gMJqJL6!!J1>/1815-/*!

)882+*!(-3!;))/!+)j:1+)9!*2!)3*-;.13(!-!52,,2/!9-*-!1/*)+5(-/>)!82+,-*6!!E/!-991*12/!*()!52,4.)*)!,29).!

,:3*!;)! *:+/)9!20)+! *2!RMJM!82+! 1/*)>+-*12/! 1/*2! *()1+!20)+-..!,29).!28! *()! 34-5)! 3*-*12/6! !M! +)9:5)9!

0)+312/!28! *(13!,29).! 13!4+2019)9!;=!RMJM! *2!MFJ! 1/! *)+,3!28! 815*1*12:3! XFDgM'Y! KF)-/!D88)5*10)!

gM91-*12/!'),4)+-*:+)L!/29)3A!?(15(!,1,15!*()!.25-.!+-91-*10)!)/01+2/,)/*!82+!*()!$&Z!5-3)36!!!

M!31,4.)!)@-,4.)!28!*()!,29).1/>!13!3(2?/!1/!H1>:+)!"6$Z&!82+!*()!*),4)+-*:+)!28! *()!?-..3!28!

2/)!'#I+-*)!.25-*)9!2/!*()!:44)+!42+*!319)!28!*()!,-1/!+-,!+-91-*2+!9:+1/>!1*3!?2+3*!(2*!24)+-*1/>!5-3)6!!

'()!?-..!*),4)+-*:+)3!-+)!?1*(1/!*()!9)31>/!+)j:1+),)/*36!!!

!

T crate RAM, Port50

orbital position

20

25

30

35

40

45

0 2 4 6 8 10 12 14

tem

pe

ratu

re [

°C]

T crate RAM, Port50

orbital position

20

25

30

35

40

45

0 2 4 6 8 10 12 14

tem

pe

ratu

re [

°C]

20

25

30

35

40

45

0 2 4 6 8 10 12 14

tem

pe

ratu

re [

°C]

!!

Figure 2.198: Model results for the indicated T-Crate.

!

M!.2/>!*)+,!-/-.=313!?-3!-.32!4)+82+,)9!:31/>!*()!34-5)!3*-*12/!XF1/1,:,!S+24:.312/!M**1*:9)YA!

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vacuum case temperatures while in Minimum Propulsion Attitude: various

points on main wake radiator (a), various points on main ram radiator (b),

mean of tracker wake radiator (c), mean of tracker ram radiator (d), mean

of zenith radiator (e), mean of vacuum case (f).

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2.10 Integration

The elements of the AMS-02 detector are assembled as shown in Figure 2.201 (“ram” refers to

the ISS direction of flight, “wake” is opposite, “port” and “starboard” are transverse). The assembly takes

place at a dedicated facility installed at CERN, with support from the entire collaboration, as indicated in

Figure 2.202.

As shown in Figure 2.203, after all elements are integrated, the detector is calibrated in particle

beams at CERN and GSI, Darmstadt for calibration. The detector undergoes a complete thermal vacuum

test at the ESA Large Space Simulator at ESTEC, Noordwijk, the Netherlands.

After the instrument has been completely checked out it will be partially disassembled for

transport and shipped to the Kennedy Space Center. There, after reassembly, it will be subjected to tests

to verify that it is compliant with the NASA mechanical and electrical interfaces for both the space shuttle

and the space station.

The experiment will then be installed in the shuttle and launched to the space station.

Assembly begins when Space Cryomagnetics delivers the completed and tested Magnet system,

and the NASA Mission Management Office, supported by Lockheed Martin, delivers the unique support

structure (USS) to CERN. The unique support structure is made up of three components: The USS main

beam structure, the magnet vacuum case, and the lower USS. The vacuum case will have already been

incorporated in the magnet system.

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Figure 2.201: AMS-02 Assembly (Ram - ISS flight direction).

Imaging

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2.10.1 USS and Magnet

The first step is bolting and pinning the USS main beam structure to the eight interface flanges of

the magnet vacuum case forming the main USS structure (Figure 2.204). This structure is then mounted

into a rotating and height adjustable assembly stand designed to hold AMS at the shuttle mechanical

interfaces (trunnions). The magnet support boxes (the Cryomagnet Avionics Box (CAB), Cryo-valve box

(CVB) and uninterruptible power source (UPS)) are mounted to the wake side of the USS and all

interconnections between magnet and boxes are made.

Figure 2.204: Main USS-02 structure and Magnet.

Magnet

USS-02

UPS

CAB

CVB

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2.10.2 Anticoincidence Counters (ACC)

The first detector to be installed is the anticoincidence counter (ACC). It is composed of 16

scintillator paddles each individually mounted to the inner bore of the magnet Vacuum Case (VC). Once

all paddles, fiber light guides and photomultiplier units have been inserted and mounted, they are secured

with a carbon fiber composite cylinder (see Figure 2.205).

Figure 2.205: ACC installed.

ACC

VC

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2.10.3 Tracker & Star Tracker

Next, the tracker together with the star tracker is installed. The partially assembled tracker

consisting of the cylindrical midsection with inner planes mounted together with the upper conical flange

and star tracker structure and the upper four compliant tracker feet, which structurally connect the tracker

to the Vacuum Case (VC), are lowered into the inner bore of the VC. The compliant tracker feet resting

on the VC are then bolted. The lower conical flange is bolted to the tracker cylinder and another four

compliant feet bolt to the tracker securing the lower end of the tracker to the VC. A large volume of

cables from the inner silicon planes that were rolled and bundled for installation are now routed over the

vacuum case to the 8 respective tracker crates (see Figure 2.206).

Figure 2:206: Tracker & Star Tracker with Electronics Boxes.

Next the tracker cooling system is installed. The tubing loops for cooling the inner planes and the

two outer planes are inserted and attached to the front end electronics using a precision jig. The two boxes

containing the “Tracker cooling box” and electronics are mounted on the wake side of the USS.

Condensers that are to be attached to the backside of the tracker radiators are jigged in place and all

tubing interconnecting the above components is routed and welded using a precision orbital welding

machine.

Following this the upper and lower planes of the tracker are placed on the conical tracker flanges

and bolted in place. The star tracker camera module is then bolted at the outer edge of the upper tracker

plane and to the already installed star tracker structure.

Most electronics boxes are arranged and interlinked into rack-like structures that are mechanically

self-supporting when complete. The tracker crates are the first to be installed within this self supporting

arrangement and, due to their close proximity to the main USS, are the structural links to the USS (dark

blue boxes near USS in Figure 2.206). These are installed together with a jig (not shown) that will hold

most of other boxes in place during assembly.

Star Tracker Tracker Electronics Crates

Tracker

VC

VC Flanges

Tracker Cooling Box

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2.10.4 Time of Flight (TOF) detector

The time of flight detector (TOF) is composed of two parts: the upper TOF containing two

scintillator panel layers above the tracker, and another identical set of panel layers bellow the tracker, but

supported by a different structure.

The upper TOF shares common attachment brackets with the TRD. First, they are bolted to the 4

interface flanges of the USS and then the TOF support arms are bolted to them, see Figure 2.207.

Figure 2.207: Upper and Lower Time of Flight Detectors (TOF).

Upper TOF

Lower TOF

TOF Support Arms

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2.10.5 Transition Radiation Detector (TRD)

The Transition Radiation Detector is installed by placing the corner of the TRD truss structure on

the TOF common bracket and pinning and bolting it in place. The TRD gas supply and circulation

system is hoisted and bolted to the upper wake, port side of the main USS structure. The 3mm diameter

gas lines are routed to the detector, respective electronics boxes mounted and cabling routed. The TRD

multi-layer insulation (MLI) enclosure is now wrapped and sealed around both the TRD and upper TOF

detectors, see Figure 2.208.

Figure 2.208: TRD installed with MLI enclosure.

TRD TRD MLI

TRD GAS

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2.10.6 RICH

The lower USS supporting the RICH and ECAL detectors are initially integrated separately from

the rest of the experiment. The RICH detector is lowered onto the square structure where eight brackets

secure it to the lower USS (Figure 2.209). Corresponding electronics crates are bolted to the radial arms

and cables routed.

(a) Preassembly view (b) Assembled

Figure 2.209: Lower USS-02 with RICH and ECAL.

2.10.7 ECAL

To install the ECAL, the Lower USS with the RICH already attached is lifted and lowered onto

the ECAL. The ECAL interfaces to the lower USS at the 4 corners of the square beam section

(Figure 2.209). Again electronics are mounted on the radial corner beams and cabling routed.

RICH

Lower USS

ECAL

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2.10.8 Integration of the Upper and Lower Parts

The lower USS-02 part (carrying the RICH and the ECAL) is integrated with the Upper USS-02

part. The assembled and tested lower detectors and lower USS are rolled underneath the AMS upper part,

crane lifted into position, and pinned and bolted into place. Electrical connections and testing follows,

(see Figure 2.210).

Figure 2.210: The Lower USS-02 integrated with the Upper USS-02.

Upper Part

Lower Part

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2.10.9 Radiators & Electronics

For the installation of the main radiators, each is lifted in from below, positioned and then bolted

to the crate structure. All electronics boxes are then grounded to the radiator via dedicated bonding straps,

see Figure 2.211.

Figure 2.211: Radiators installed.

After the main ram and wake radiators have been installed, the GPS electronics box is mounted to

the upper inside, ram, radiator and the GPS antennas bolted to the upper, ram, starboard, trunnion beam of

the USS. Then the system is electrically interconnected and connected to rest of AMS.

Tracker radiators are then installed, lifting them into place and bolting the strut structures to the

upper USS and vacuum case joints. The tracker cooling heat exchanger is bolted to the radiator and the

jigs holding them removed.

The Zenith radiator, located on top of the TRD, is installed last. The radiator is composed of four

quadrants, each panel cooling one of the four cryocoolers. Each radiator panel, with the lengthy pre-bent

3mm tubing and attached heat exchangers, is lowered onto the TRD. The tubing is then secured to

designated bracketry and the heat exchangers bolted to their respective cryocoolers.

RAM Radiator

WAKE Radiator

Tracker Radiator

Tracker Radiator

Zenith Radiator

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2.10.10 ISS Hardware

At Kennedy Space Center AMS will be fully completed with the addition of shuttle and ISS

hardware. There, the USS Keel, and interface with shuttle and ISS will be installed (Figure 2.212).

Figure 2.212: Complete assembly including shuttle & ISS hardware.

A full-scale mock up of AMS-02 has been built at CERN to develop and verify the assembly

procedure, see Figure 2.213.

Figure 2.213: AMS-02 full-scale mock-up.

ISS Hardware

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2.11 Operations

The operations of the AMS-02 experiment are divided into five distinct phases: Prelaunch, Ascent,

STS on orbit, Transfer from STS to ISS and ISS on orbit. The AMS Crew Operations Post (ACOP) will

have been launched to the station on a previous flight. During the intervening months it will be installed

in the US Lab of the ISS and checked out to be ready for the arrival of AMS.

2.11.1 Prelaunch Operations

After the experiment has been turned over to NASA at KSC for processing, it is installed in the

shuttle payload bay. Flight power and data connections to the shuttle are made via the Remotely

Operated Electrical Umbilical (ROEU), see Figure 2.1. For prelaunch operations connections are also

made through the ROEU to the tail of the shuttle and out through T-0 umbilical to equipment in the

Mobile Launch Platform (MLP) underneath the shuttle. The flight connections are checked with a series

of Interface Verification Tests (IVT) and End to End Tests.

During this prelaunch phase a vent pump mounted on AMS continuously removes boil off from

the helium vessel. In addition, by using ground support computers located in the MLP, personnel

monitor the 1553 Bus data for telemetry including temperature and pressure measurements and cryogenic

system operating characteristics. The health and status of the Super Fluid Helium (SFHe) Tank are

monitored by ground controllers and compared to established trend data. Depending on the thermal

environment, the cryocoolers may be operational.

While on the launch pad the magnet will not be charged and is at zero field.

Shortly before the shuttle payload bay doors are closed at launch minus a few days, the cryogenic

ground support equipment is used to top off the SFHe tank (§ 2.1.3.ix).

At launch minus 30 minutes, power to AMS over the T-0 is reduced to an absolute minimum and

the vent pump turned off and the vent valve sealed.

Monitoring of the cryogenics and vacuum continue until at least launch minus nine minutes at

which time ground controllers make a “Go/No Go” decision for launch based on the health and status of

the SFHe Tank. After that, power to AMS may be cut off completely.

At launch, the T-0 umbilical is disconnected and control passes from KSC to JSC.

2.11.2 Ascent

While still under powered flight but when the pressure in the payload bay has approached zero

(less than 20 mbar), a barometric switch opens a vent valve on the SFHe tank. This ensures that the

superfluid helium is not in contact with the passive phase separator. The barometric switch is backed up

with a time-tagged command issued from the shuttle Backup Flight System General Purpose Computer.

In the event of an ascent abort, the barometric switch will close the vent valve.

2.11.3 STS on orbit operations

Once on-orbit, the payload bay doors are opened. At about 2.5 hours after launch, AMS receives

power from the APCU power supply and communication is established between AMS, the Digital Data

Recording System (DDRS-2) in the orbiter and the ground. Control and monitoring of the cryogenics

systems is reestablished and the cryocoolers activated. The subdetector elements are then checked out,

either one by one or altogether, depending on thermal conditions. The magnet cannot be charged (see

Figure 2.158) and remains at zero field. This continues for a couple of days until the shuttle approaches

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the ISS, when certain key cryogenics valves are operated. After thermal conditioning, AMS is powered

off.

2.11.4 STS to ISS transfer

Transfer operations commence when the space shuttle arm (SRMS) latches on to Flight

Releasable Grapple Fixture (FRGF) mounted on AMS. Then the ROEU is disconnected, the Payload

Retention Latch Actuators (PRLAs) and Active Keel Attachments are opened releasing the trunnions, and,

as shown in Figure 2.214, the shuttle arm lifts AMS out of the shuttle payload bay. It is then maneuvered

towards the space station where the station arm (SSRMS) latches on to the Power and Video Grapple

Fixture (PVGF). The hand off is completed when the shuttle arm is disengaged. Power then flows

through the station arm into AMS where it is used, as needed, to operate thermostatically controlled

heaters which maintain the experiment elements in their operational ranges. The station arm then swings

AMS over to the S3 station truss and, using the Berthing Cue System cameras, docks it in the upper,

inboard payload attach site. The capture claw of the active Payload Attach System on the station then

mechanically secures AMS to the station and then the Umbilical Mechanical Assembly (UMA) is driven

activated and AMS is electrically mated to the station. Power from the arm to AMS is then cut off and

the power through the UMA is activated. As the experiment has been kept in a good thermal condition

by power from the station arm, it activates immediately and communication is established between AMS,

ACOP and the ground. Then the station arm is disengaged and transfer operations are complete. In total,

from power down in the space shuttle to power up on the space station, based on extensive simulations

run by NASA, the transfer is estimated to take less than four hours.

2.11.5 ISS On-Orbit Operations

ISS on orbit operations start with the reestablishing of the health and status of the cryogenics

system. The cryocoolers are activated. While preparations are being made for charging the magnet, the

other experiment elements are checked out and some zero field data for calibration and alignment

purposes may be taken. When the cryogenic systems are ready, all the other experimental elements are

powered down and the CCS in the CAB (see Figure 2.22) is activated and the magnet is ramped to field,

which will take two hours. Then the experimental elements are re-powered and nominal data taking

proceeds.

Though all necessary protection is in place to accommodate reduced power levels from the ISS or

even foreseen or unforeseen power outages, it is anticipated that the experiment will run continuously for

three to five years, at which point the SFHe will be exhausted and the magnet will warm up and return to

zero field. At this point the cryocoolers are turned off but, as detailed in the next section, a wealth of

interesting physics data can still be obtained.

All critical interfaces (power, LRDL, HRDL) between AMS and ISS are redundant. If necessary,

a contingency intervention (extra-vehicular activity or EVA), as shown in Figure 2.159, can be performed

by the astronauts to swap cables between the redundant units.

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Fig

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AM

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AM

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! "#$%&

2.12 AMS-02 Physics Examples '()#*"!+,--!./! 01/! 2,340!56783!9630,:-/!91;4,:4!/<9/3,5/=0!8=! 01/!)96:/!)060,8=>! !?1/!91;4,:4!

@86-4!82!'()!63/!08!4/63:1!283!6=0,5600/3!A$B!,=!01/!C=,D/34/!60!01/!-/D/-!82!$!,=!$!.,--,8=E!08!4/63:1!283!01/!

83,@,=!82!F63G!5600/3!A"BE!08!5/64H3/!01/!49/:03H5!82!1,@1!/=/3@;!@6556!36;4!6=F!08!56G/!1,@1!4060,40,:4!

5/64H3/5/=04!82!01/!:85984,0,8=!82!:845,:!36;4!H9!08!01/!5H-0,#?/I!/=/3@;!36=@/>!!!

J=! 01,4! :1690/3E! /<659-/4! 82! 01/! 91;4,:4! :696.,-,0,/4! 82! '()#*"! 63/! 93/4/=0/F>! ! ?1/4/! 40HF,/4!

+/3/!56F/!H4,=@!01/!'()#*"!4,5H-60,8=!96:G6@/!+1,:1!,=:-HF/4K!!6!F/06,-/F!F/4:3,90,8=!82!01/!'()#*"!

@/85/03;E! 6! 4,5H-60,8=! 82! 01/! :845,:! 36;! 2-H</4! .64/F! 8=! F606! :8--/:0/F! +,01! '()#*$E! 6! :859-/0/!

4,5H-60,8=!82! 01/!/D/=0!H4,=@! 01/!LM'N?!&!A&B!96:G6@/E! 6! 4,5H-60,8=!82! 01/! 03,@@/3! OP640E!Q/D/-#$!6=F!

Q/D/-#&RE!/D/=0!3/:8=403H:0,8=E!D,4H6-,S60,8=!088-4!O/D/=0!F,49-6;E!822-,=/!58=,083,=@R!6=F!088-4!283!(8=0/!

T63-8!938FH:0,8=>!!!

!

2.12.1 AMS-02 Detector Simulation

?1/!6::H360/!4,5H-60,8=!82!01/!F/0/:083!3/UH,3/4!6!:859-/0/!F/4:3,90,8=!82!01/!@/85/03;E!560/3,6-4!

6=F!3/498=4/!82!6--!01/!/<9/3,5/=0!/-/5/=04K!01/!:3;856@=/0E!01/!036=4,0,8=!36F,60,8=!F/0/:083!O?VWRE!01/!

4,-,:8=! 036:G/3E! 01/! 0,5/! 82! 2-,@10! 6=F! 6=0,:8,=:,F/=:/! 4:,=0,--60834! O?XP! 6=F! 'TTRE! 01/! 3,=@! ,56@,=@!

T/3/=G8D!F/0/:083!OVJTYR!6=F!01/!/-/:03856@=/0,:!:6-83,5/0/3!OMT'QR>!!!

?1/!4H9/3:8=FH:0,=@!56@=/0!164!01/!4169/!82!6!:;-,=F3,:6-!41/--!+,01!6=!,==/3!F,65/0/3!82!$>"!5!

6=F! 6! -/=@01! 82! *>%!5>! ! J0! 938FH:/4! 6! :/=036-! F,98-/! 2,/-F! 82! *>Z[!?/4-6! 6:3844! 01/!56@=/0! .83/>! ! ?1/!

56@=/0,:!2,/-F!569!,4!,=:-HF/F!6=F!01/!0367/:083,/4!82!9630,:-/4!,=!01/!2,/-F!63/!4,5H-60/F!,=!F/06,->!!!

?1/!?VW!,4!4,0H60/F!8=!01/!089!82!01/!49/:0385/0/3!6=F!:8=4,404!82!0+/=0;!-6;/34!82!"*!55!01,:G!

2,./3! 36F,6083! ,=0/3-/6D/F! +,01! 6336;4! 82! [!55! F,65/0/3! @64! 9389830,8=6-! 0H./4! 2,--/F! +,01! 6! \/KTX"!

5,<0H3/>! ! J0! 938D,F/4! /-/:038=]16F38=! 4/96360,8=! 60! /=/3@,/4! H9! 08! "^*!L/I! 64!+/--! 64! :163@/F! 9630,:-/!

:883F,=60/!5/64H3/5/=04>!!!

?1/!/,@10! -6;/34!82!F8H.-/!4,F/F!4,-,:8=! 036:G/3!63/!6336;/F! 036=4D/34/! 08! 01/!56@=/0!6<,4>! !?1/!

036:G/3! 5/64H3/4! 01/! 0367/:083;! 82! 4,=@-;! :163@/F! 5,=,5H5! ,8=,S,=@! 9630,:-/4! O(J_4R! +,01! 6=! 8D/36--!

6::H36:;! 82! 6.8H0! $*! `5! ,=! 01/! ./=F,=@! 9-6=/! 6=F! &*! `5! ,=! 01/! =8=#./=F,=@! 9-6=/! 6=F! 938D,F/4!

5/64H3/5/=04!82!01/!9630,:-/!/=/3@;!-844>!!!

?1/!0,5/!82!2-,@10!4;40/5!164!28H3!-6;/34!6=F!5/64H3/4!4,=@-;!:163@/F!9630,:-/!036=4,0!0,5/4!+,01!

6=!6::H36:;!82!$&*!94>!!J0!6-48!938D,F/4!/=/3@;!-844!6=F!:883F,=60/!5/64H3/5/=04>! !?1/!6=0,:8,=:,F/=:/!

4:,=0,--60834!2-6@!9630,:-/4!/=0/3,=@!83!-/6D,=@!01/!4/=4,0,D/!D8-H5/!8H04,F/!82!01/!6::/906=:/>!!!

?1/!VJTY!F/0/:083!:8=4,404!82!0+8!36F,60834!O6!&!:5!01,:G!'/38@/-!36F,6083!+,01!3/236:0,D/!,=F/<!

82!$>*&!6=F!6!:/=036-!*>^!:5!01,:G!N6P!36F,6083!+,01!6=!63/6!82!$$^[!:5"!6=F!6!3/236:0,D/!,=F/<!82!$>&aRE!6!

5,3383!6=F!6=!,56@,=@!9-6=/!5603,<!82!9,</-!0;9/!918085H-0,9-,/3!0H./4!283!-,@10!F/0/:0,8=>!!J0!644H3/4!01/!

5/64H3/5/=0!82! 01/!D/-8:,0;!82! 4,=@-;!:163@/F!(J_4!+,01! 6=! 6::H36:;!./00/3! 016=!8=/!9/3!5,-! 6=F! 01/!

6.48-H0/!56@=,0HF/!82!01/!:163@/!64!+/--!64!938D,F,=@!6=!H=65.,@H8H4!06@!82!01/!9630,:-/!2-,@10!F,3/:0,8=!

OH9+63F4!83!F8+=+63F4R>!!!

?1/! MT'Q! ,4! 6! &W! /-/:03856@=/0,:! 4659-,=@! :6-83,5/0/3! +,01! 0806-! 82! $[>b! 36F,60,8=! -/=@014!

56F/!82!$!55!F,65/0/3!4:,=0,--60,=@!2,./34!46=F+,:1/F!./0+//=!@388D/F!-/6F!9-60/4>!!!

?1/!4,5H-60/F!9/328356=:/!82!01/!'()!4H.F/0/:0834!+64!:1/:G/F!6@6,=40!01/!'()#*$!2-,@10!6=F!

6@6,=40! 0/40! ./65! F606! 6=F! 28H=F! 08! ./! ,=! @88F! 6@3//5/=0>! ! J=! 6FF,0,8=E! 08! 4,5H-60/! 3/6-! F/0/:083!

9/328356=:/!620/3!&!;/634!8=!J))E!$!08!"!9/3!:/=0!82!01/!4H.F/0/:083!3/6F8H0!:16==/-4!+/3/!644H5/F!F/6F>!!

?1/!4,5H-60/F!/D/=04!+/3/!03,@@/3/F!.;!01/!:8,=:,F/=:/!82!4,@=6-4!,=!013//!8H0!82!28H3!?XP!9-6=/!6=F]83!

4,@=6-4!,=!01/!/-/:03856@=/0,:!:6-83,5/0/3>!!!

?8! /=4H3/! 6! F/06,-/F! /D6-H60,8=! 82! 01/! '()#*"! 91;4,:4! 9/328356=:/E! 583/! 016=! $*$*! /D/=04E!

,=:-HF,=@! 93808=4E! /-/:038=4E! 984,038=4E! F/H0/38=4E! 6=0,93808=4E! Y/! 6=F! 801/3! 1/6D,/3! =H:-/,E! 63/! ./,=@!

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!"#$%a!

4,5H-60/F! 60! F,22/3/=0! /=/3@,/4>! ! ?8! 6:1,/D/! 01,4! @86-! 6! :8--6.8360,8=!+,F/! /22830! 164! .//=! H=F/306G/=>!!

P,@H3/!">"$^!418+4!01/!"$!(8=0/#T63-8!938FH:0,8=!:/=0/34>!!?1/!:H33/=0!:696:,0;E!64!5/64H3/F!FH3,=@!6!

-8=@! 0/35! O$**! F6;R! 938FH:0,8=! 3H=E! ,4! 0160! "!<!$*b! /D/=04! O583/! 016=! &*! Lc;0/R! :6=! ./! 4,5H-60/FE!

:8--/:0/F! 6=F! 3/F,403,.H0/FE! 8=! 6D/36@/E! /6:1! F6;>! ! ?1/! /<9/3,5/=06-! 4/=4,0,D,0;! 40HF,/4! 93/4/=0/F! 63/!

.64/F!8=!01/4/!4060,40,:4>!!!

!

!!

Figure 2.215: AMS Monte Carlo Production and Regional Analysis Centers.!!M6:1!:/=0/3!9630,:,960/4!

,=! 938D,F,=@! F,403,.H0/F! :859H0,=@! 3/48H3:/4E! 3/580/! 4820+63/! F/D/-895/=0! 6=F! 91;4,:4!

6=6-;4,4E! =/+! 4820+63/! 088-4! 283! =/0+83G,=@! 6=F! ,=0/3938:/44! :855H=,:60,8=! 6=F! 6!

+83G,=@!938080;9/!82!01/!@38H=F!F606!16=F-,=@!283!01/!'()#*"!5,44,8=>

2.12.2 Antimatter search

?1/!56,=!.6:G@38H=F4! 08!6!@/=H,=/! /Y !4,@=6-!63/!Y/!/D/=04!+1,:1!63/!/,01/3!5,45/64H3/F!83!

+1,:1!,=0/36:0/F!,=!01/!'()!F/0/:083>! !C4,=@!6!4/-/:0,8=!938:/FH3/!4,5,-63! 08!0160!H4/F!,=!01/!'()#*$!

6=0,5600/3! 4/63:1E! 01/! 6D/36@/!'()#*"! 6::/906=:/! 283! /Y ! /D/=04!+64! /40,560/F! 08! ./! *>a!5"43>! ! ?1/!

4/-/:0,8=!/22,:,/=:;!283! /Y !D63,/4!2385!b*d!O2385!"!08!$**!LIR!08!&d!O638H=F!$!?IR>! !N8!Y/!/D/=04!

4H3D,D/!01/!:H04>!!_387/:0,=@!01,4!3/4H-0!08!6!&!;/63!5/64H3/5/=0E!6! /Y ]Y/!-,5,0!82!83F/3!82!$*!%!+,--!./!

8.06,=/F!283!3,@,F,0,/4!H9!08!$&*!$a*!LI!OP,@H3/!">"$[R>!

!

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! "#$%^

10-9

10-8

10-7

10-6

10-5

10-4

10-3

10-2

1 10 102

103

An

tihe

lium

/He

lium

Flu

x R

atio

(9

5%

C.L

.)

Rigidity (GV)

(a) Buffington etal. 1981

(b) Golden etal. 1997

(c) Badhwar etal. 1978

(d) Alcaraz etal. 1998

(e) Sasaki etal. 2001

(a)

(b)(c)

(c)

(d)

(e)

AMS-02 3 Years

!!

Figure 2.216: Projected AMS-02 limits on the eH /He flux ratio compared to

previous measurements [4] including AMS-01 (d).

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!"#$%[!

2.12.3 Dark matter search using the positron spectrum

'::83F,=@!08!)C)e!01/83,/4E!01/!-/6F,=@!F63G!5600/3!:6=F,F60/!,4!01/!=/H036-,=8E! ! >!!N/H036-,=8!6==,1,-60,8=!,=!01/!@6-6:0,:!16-8!:6=!938FH:/! 9 E!/f!6=F!$!D,6K!!!

# !#%#!#&# 9 + ..."##

# & /+ +...,!

! & $ +... 6=F

# &#W +...

?1/! 9 E!/f!6=F!$!2385!01/4/!:8--,4,8=4!938FH:/!F/D,60,8=4!2385!458801!/=/3@;!49/:036!A^B>!?1/3/283/E!01/!

93/:,4,8=! 6=F! 4,5H-06=/8H4!5/64H3/5/=0! 82! 01/! 9 ,! /fE! $! 6=F! W ! 49/:036!A[B!+,--! /=6.-/! H4! 08! /406.-,41!+1/01/3!)C)e!9630,:-/4! O283! /<659-/!=/H036-,=84R! 63/! 01/!83,@,=! 82!W63G!(600/3>! !?1/! /<659-/! ,=! 01,4!

4/:0,8=!:8=:/=0360/4!8=!984,038=4>!

?+8!58F/4! 63/!H4/F! 08!F/0/:0!984,038=4>! !c801!H4/! 01/!?VW!283! /-/:038=]93808=!F,4:3,5,=60,8=!

6=F!01/!?XPf?36:G/3!283!:163@/!56@=,0HF/!6=F!4,@=!F/0/35,=60,8=>!!?1/!low energy mode!3/-,/4!8=!01/!

VJTY! 283! 01/! D/-8:,0;! 5/64H3/5/=0! +1,-/! high energy mode! H4/4! 01/! MT'Q! 08! 2H301/3! ,5938D/! 01/!

4/-/:0,8=!82!984,038=4!2385!01/!16F38=,:!.6:G@38H=F4>!!C4,=@!01/4/!0+8!58F/4!8D/36--!3/7/:0,8=!26:0834!82!

./00/3!016=!$]$*[!6@6,=40!93808=4!6=F!$]$*a!6@6,=40!/-/:038=4!16D/!.//=!8.06,=/F!AbB>!!?1,4!6--8+4!6!:-/6=!

5/64H3/5/=0!82!01/!984,038=!49/:03H5!H9!08!&^*!L/I>!!P,@H3/!">"$b!418+4!01/!(8=0/!T63-8!:85963,48=!

./0+//=! 01/! @/=/360/F! 6=F! 3/:8=403H:0/F! 49/:036>! ! P,@H3/!">"$Z! 418+4! 01/! 6=0,:,960/F! '()#*"!

5/64H3/5/=0!82!01/!984,038=!49/:03H5!,=!01/!93/4/=:/!82!F63G!5600/3!6==,1,-60,8=>!!!

!!

Figure 2.217: Secondary positron spectrum comparison predicted for AMS-02 .

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! "#$%b

!!

Figure 2.218: An example of AMS-02 positron spectrum measurement in the

absence (a) or presence (b) of a neutralino with mass !m = 130 GeV.

2.12.4 Dark matter search using the antiproton spectrum

?1/!56,=!.6:G@38H=F4!08!01/!6=0,93808=!4,@=6-!63/!93808=!6=F!/-/:038=!/D/=04>!!V/7/:0,8=!26:0834!

./00/3! 016=! $*[! 6=F! $*&! 63/! :833/498=F,=@-;! =//F/F! 08! 6--8+! 01/! .6:G@38H=F! 23//!5/64H3/5/=0! 82! 01/!

6=0,93808=!49/:03H5!H9!08!/=/3@,/4!82!6!2/+!1H=F3/F!L/I>!!

?1/! 93808=! .6:G@38H=F! +64! 3/7/:0/F! H4,=@! 01/! 3,@,F,0;! 5/64H3/5/=0! ,=! 01/! 036:G/3E! +1,-/! 01/!

?VWE! VJTY! 6=F! MT'Q! +/3/! H4/F! 08! 3/7/:0! /-/:038=4>! ! P,@H3/!">"$%! 418+4! 01/! 3/7/:0,8=! 26:0834!

8.06,=/F!AZB>!!P,@H3/!">""*!418+4!01/!4,5H-60/F!6=0,93808=!49/:03H5!5/64H3/5/=0!8.06,=/F!+,01!'()#*"!

,=!&!;/634!82!F606!06G,=@>!!!

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!"#$%Z!

!!

Figure 2.219: Estimated proton (left) and electron (right) rejection factors

for the AMS-02 antiproton flux measurement.

!!

Figure 2.220: Example of a AMS-02 antiproton flux measurement

together with recent experimental data [9].

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! "#$%%

2.12.5 Gamma ray spectra

_3/:,4/!5/64H3/5/=0!82!F,22H4/!@6556!36;!2-H</4!56;!6-48!3/D/6-!01/!83,@,=!82!F63G!5600/3E!+1,-/!

@6556! 36;4! 83,@,=60,=@! 2385! F,22/3/=0! 48H3:/4! 4H:1! 64! 6:0,D/! @6-6:0,:! =H:-/,! O'LNR! 6=F! @6556! 36;!

.H3404!56;!938D,F/!,=283560,8=!6.8H0!9844,.-/!UH6=0H5!@36D,0;!/22/:04>!!'()#*"!+,--!./!6.-/!08!5/64H3/!

01/!@6-6:0,:!6=F!/<036@6-6:0,:!F,22H4/!@6556!36;!49/:036!H9!08!$!?/I!A$*B>!!J=!6FF,0,8=E!H9!08!$*!@6556!

36;!.H3404!6=F!6.8H0!^**!'LN!9/3!;/63!+,--!./!3/:83F/F>!!!

?1/!56,=!.6:G@38H=F4!08!@6556!36;!4,@=6-4!63/!01/!93808=!6=F!/-/:038=!O984,038=R!/D/=04>!!?+8!

F,40,=:0!@6556!36;!4,@=60H3/4!+/3/!/<9-8,0/F!08!/40,560/!01/!:696.,-,0;!82!'()#*"!08!F/0/:0!@6556!36;4K!

-8+!/=/3@;!58F/!6=F!1,@1!/=/3@;!58F/>!

J=! -8+! /=/3@;!58F/E! 01/! 91808=! ,4! :8=D/30/F! ,=! 089! 82! '()! 6=F! 6=! /-/:038=#984,038=! 96,3! ,4!

F/0/:0/F! ,=! 01/!'()!036:G/3!>! !?1,4!5/018F!82!40HF;,=@!:845,:!(! 36;4! ,4! 4,5,-63! 08! 01/!5/018F!H4/F!60!

WM)e!08!40HF;!$!f!N!&!N!f!/f/!! 3/6:0,8=4!A$$B>! !P385!01/!5/64H3/5/=0!82! 01/!938FH:0,8=!6=@-/4!6=F!/=/3@,/4!82! 01/!/fE!/!!96,3E!gMW!938D,F/4!/<:/--/=0! ,=283560,8=!8=!01/! ,=,0,6-!F,3/:0,8=!82!(! 36;>! ! J=! 01,4!

58F/! 91808=4! 56;! ./! F/0/:0/F! 2385! $! 08! "**!L/I! +,01! /<:/--/=0! 98,=0,=@! 6::H36:;E! 418+=! ,=!

P,@H3/!">""$>!!!

Energy (GeV)

! R

esol

utio

n (°

)

1 10 102

Figure 2.221: Estimated AMS-02 photon angular resolution vs. energy.

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!"#"**!

J=!1,@1!/=/3@;!58F/E! 01/!91808=! ,4!F/0/:0/F!.;! ,04!:1636:0/3,40,:! 418+/3! ,=! 01/!/-/:03856@=/0,:!

:6-83,5/0/3!6=F!6=!6.4/=:/!82!:163@/F! 036:G4! ,=! 01/! 3/40!82! 01/!F/0/:083>! ! J=! 01,4!58F/!91808=4!56;!./!

F/0/:0/F! 2385!6! 2/+!L/I!H9! 08!?/I!+,01!6=!/=/3@;!3/48-H0,8=!82!6! 2/+!9/3!:/=0!6=F!6! 0;9,:6-!6=@H-63!

3/48-H0,8=! 82! $! F/@3//>! ! P,@H3/!">"""! 418+4! 01/! (8=0/! T63-8! :85963,48=! ./0+//=! 01/! @/=/360/F! 6=F!

3/:8=403H:0/F!49/:036!82!@6-6:0,:!6=F!/<036@6-6:0,:!(!36;4!H9!08!/=/3@;!82!$!?/I>!

!

Energy (GeV)

" (D

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(m-2

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Measured SpectrumInitial SpectrumBackground

10-3

10-2

10-1

1

10 102 103

Energy (GeV)

Measured SpectrumInitial SpectrumBackground

0.002

0.004

0.006

0.008

0.01

0.012

0.014

0.016

0.018

0.02

10 102 103

" (E

xtra

Gal

) Flu

x (m

-2 sr

-1 se

c-1 G

eV)

!!

Figure 2.222: Projected AMS-02 measurements of the diffuse galactic (left) and extra-

galactic (right) gamma flux [7]. Photons up to 1 TeV will be detected.

!

2.12.6 Cosmic Ray Spectra

'()#*"!+,--!93/:,4/-;!F/0/35,=/!01/!2-H</4!82!,=F,D,FH6-!/-/5/=04!+,01!:163@/!56@=,0HF/!60!H9!

08!60! -/640!"[! OP/R! ,=! 01/!/=/3@;! 36=@/! 2385!$**!(/I]=H:-/8=! 08!$!?/I]=H:-/8=>! !P,@H3/4!">""&E!">""a!

6=F!">""^!418+!01/!9387/:0/F!'()#*"!5/64H3/5/=04!82!01/!93808=E!/-/:038=!6=F!Y/!2-H</4!A$"B>!!!

J=F/9/=F/=0-;!82!01/!56@=/0!6=F!4,-,:8=!036:G/3E!-8+!6=F!1,@1!/=/3@;!96304!82!:845,:!36;!49/:036!

+,--!6-48!./!5/64H3/F!.;!01/!VJTY!6=F!?VW!3/49/:0,D/-;>! !P,@H3/4!">""[!6=F!">""b!418+!01/!'()#*"!

5/64H3/5/=04!82!01/!:63.8=!49/:03H5!H4,=@!01/!VJTY!6=F!82!01/!,38=!49/:03H5!.64/F!8=!01/!?VW!F606>!!!

Y,@1! 4060,40,:4! 5/64H3/5/=04! 82! 01/! 1/6D;! =H:-/,! F/0/:0/F! .;! '()#*"! +,--! 6--8+! 01/! 93/:,4/!

5/64H3/5/=0!82!01/!.838=!08!:63.8=!360,8E!64!418+=!,=!P,@H3/!">""Z>!!!

!

Page 233: 2004 Ams Nim Paper Draft

AMS-02/Physics

! "#"*$

Kinetic Energy (GeV)

Pro

ton

Flux

(m2

sr se

c M

eV)-1

10-8

10-7

10-6

10-5

10-4

10-3

10-2

10-1

1 10 102 103

!!

Figure 2.223: Projected AMS-02 proton flux measurement

in 1 week (statistical errors not visible).

!

Page 234: 2004 Ams Nim Paper Draft

AMS-02/Physics

!"#"*"!

Kinetic Energy (GeV)

Ele

ctro

n Fl

ux (m

2 sr

sec

MeV

)-1

10-10

10-9

10-8

10-7

10-6

10-5

10-4

10-3

10-2

10-1

10 -1 1 10 102 103

!!

Figure 2.224: Projected AMS-02 measurement of the electron cosmic ray spectrum over 3 years.

!

Page 235: 2004 Ams Nim Paper Draft

AMS-02/Physics

! "#"*&

Kinetic Energy (GeV/N)

He

Flux

( m

2 sr s

ec M

eV/N

)-1

10-9

10-8

10-7

10-6

10-5

10-4

10-3

10-2

1 10 10 2 10 3

!!

Figure 2.225: Projected AMS-02 measurement of the He flux over 1 month.

!!

Page 236: 2004 Ams Nim Paper Draft

AMS-02/Physics

!"#"*a!

Kinetic Energy (GeV/N)

C F

lux

(m2 s

r sec

MeV

/N)-1

10 -6

10-5

10-4

10-3

10-2

10-1

1 10

Figure 2.226: Projected AMS-02 10 day measurement of the carbon flux using the RICH.

This measurement may be performed with the magnet at zero field.

Page 237: 2004 Ams Nim Paper Draft

AMS-02/Physics

! "#"*^

Kinetic Energy (GeV/N)

Fe F

lux

(m-2

sr-

1 se

c-1

(GeV

/N)-1

)

!

Figure 2.227: Projected AMS-02 1 year measurement of the iron flux using the TRD.

This measurement may be performed with the magnet at zero field.

!

Page 238: 2004 Ams Nim Paper Draft

AMS-02/Physics

!"#"*[!

Kinetic Energy (GeV/n)

B / C

Strong & Moskalenko

Dwyer et al.

HEAO-3

ISEE-3

Spacelab-2

AMS-02 (6 months)

0

0.1

0.2

0.3

0.4

10-1

1 10 102

103

Figure 2.228: Projected AMS-02 6 month measurement of the Boron to Carbon ratio,

together with recent data from different experiments [13].

Page 239: 2004 Ams Nim Paper Draft

AMS-02/Physics

! "#"*b

2.12.7 Search for anomalously heavy nuclei

NH5/38H4!4/63:1/4!283!6=856-8H4-;!1/6D;!=H:-/,!,=!:845,:!36;4!6=F!,=!01/!6058491/3/!16D/!.//=!

:8=FH:0/F!8D/3!01/!9640!;/634!H4,=@!.6--88=!6=F!460/--,0/#.83=!/<9/3,5/=04!64!+/--!64!-64/3!49/:0384:89;!

6=F!@/84,458-8@;!A$aB>!!'!2/+!:6=F,F60/!/D/=04!16D/!.//=!28H=F!6=F!-,5,04!8=!01/!9844,.-/!2-H<!82!4H:1!

/D/=04!/406.-,41/F>! !X=/!82! 01/!580,D60,8=4! 283!4H:1!4/63:1/4! ,4! 01/!9844,.-/!/<,40/=:/!82!4036=@/!UH63G!

5600/3!,=!01/!2835!82!4036=@/-/04!A$^B>!!C4,=@!583/!016=!28H3!5,--,8=!Y/!/D/=04!:8--/:0/F!+,01!01/!'()#

*$! F/0/:083! FH3,=@! 01/! )?)#%$! 2-,@10! ,=! hH=/! $%%ZE! 6! 4/63:1! +64! 9/32835/F! 283! F8H.-;! :163@/F!

6=856-8H4-;! 1/6D;! =H:-/,!A$[B>! ! '4! 418+=! ,=! P,@H3/!">""%E! 8=/! /D/=0! :6=F,F60/! +64! 28H=F! +,01! i]'!

638H=F!*>$$>!!?1/!.6:G@38H=F!938.6.,-,0;!82!4H:1!/D/=0!,4!/40,560/F!60!*>$d>!!j,01!01/!-63@/!6::/906=:/!

82!'()#*"!6=F!583/!016=!$E***!F6;4!82!F606!:8--/:0,8=E!!'()#*"!+,--!./!6.-/!08!F/0/:0!583/!016=!"**!

4H:1!/D/=04!6=F!F,4:8D/3!4036=@-/04!,2!01/;!/<,40>!!!

!

!!

Figure 2.229: Measurement of Z/A using AMS-01 data for selected He events.

Page 240: 2004 Ams Nim Paper Draft

AMS-02/Physics

!"#"*Z!

2.12.8 Measurement of 10

Be/9Be ratio

?1/!D/-8:,0;!3/48-H0,8=!82!01/!VJTY!5/64H3/F!+,01!0/40!./654!:6=!./!4//=!,=!P,@H3/!">$"b>!!?1,4!

,59-,/4!6=!/<:/--/=0!:696.,-,0;!283!'()#*"!08!4/96360/!./3;--,H5!,48089/4>! !?1,4!6.,-,0;! 08!56G/!6!1,@1!

4060,40,:4!F/0/35,=60,8=!82!01/!$*c/]%c/!360,8!+8H-F!/=6.-/!'()#*"!08!9/32835!8=/!82!01/!5840!,598306=0!

5/64H3/5/=04!,=!:845,:!36;!91;4,:4K!6!1,@1-;!6::H360/!F/0/35,=60,8=!82!01/!:845,:!36;!:8=2,=/5/=0!0,5/!

,=! 01/!@6-6<;!6=F!6!F/0/35,=60,8=!82! 01/!5/6=!F/=4,0;!82! ,=0/340/--63!560/3,6-! 036D/34/F!.;!:845,:!36;4>!!

P,@H3/!">"&*!418+4!01/!3/4H-0!9387/:0/F!H4,=@!01/!'()#*"!VJTY!8D/3!8=/!;/63!82!F606!06G,=@>!!!

!

Kinetic Energy (GeV/n)

10B

e / 9

Be

Strong & Moskalenko

ACE

Ulysses

ISOMAX

Voyager

ISEE-3

AMS-02 (1 year)

0.070.080.09

0.1

0.2

0.3

0.4

0.5

0.6

10-1

1 10

!!

Figure 2.230: Projected AMS-02 1 year measurement of the 10

Be / 9Be ratio energy

dependence compared with a diffusion/convection model prediction

(curve) together with the results from satellite measurements [17].

Page 241: 2004 Ams Nim Paper Draft

AMS-02/Physics

! "#"*%

2.12.9 References

A$B! '>W>!)6G1638DE!hM?_!Q/00/34!5!O$%[bR!"ak!'>W>!W8-@8D!6=F!e6>c>!i/-F8D,:1!et al.E!V/D>!(8F>!_1;4>!53!O$%Z$R!$k!

M>j>!l8-.!6=F!(>)>!?H3=/3E!'==>!V/D>!NH:->!_630>!):,>!33!O$%Z&R![a^k!

'>W>!W8-@8DE!_1;4>!V/9>!222!O$%%"R!&*%k!

W>!T85/--,!et al.E!NH:->!_1;4>!B412!O$%%aR!aa$k!

'>W>!W8-@8D!6=F!h>!),-GE!_1;4>!V/D>!D47!O$%%&R!a"aak!

(>eH>!l1-898DE!L36D,060,8=!6=F!T8458-8@;!4!O$%%ZR![%#b"k!

'>L>!T81/=!et al.E!'9>!h>!495!O$%%ZR!^&%#^a%k!

h>!V/15!6=F!l>!h/F65S,G!et al.E!_1;4>!V/D>!Q/00>!81!O$%%ZR!&&*b#&&$*k!

'>W>!W8-@8DE!Q/:>60!"^01!J?M_!j,=0/3!):188-E!O$%%bRE!1/9#91]%b*ba$%k!

j>!l,==/;!et al.E!_1;4>!V/D>!Q/00>!79!O$%%bR!"["*k!

(>eH>!l1-898D!et al.E!_1;4>!V/D>!D62!O"***R!Z&#^*^k!

h>!V/15!6=F!l>!h/F65S,G!et al.E!O"***R!63\,DK64038#91]***[&Z$>!

A"B! Q>c/3@403m5E!V/9>!_38@>!_1;4>!63O"***R!b%&#Za$k!

h>!M--,4!et al.E!_1;4>!Q/00>!B214 O$%%ZR!&k!

(>!?H3=/3!6=F!P>!j,-:S/GE!_1;4>!V/D>!D42!O$%%*R!ak!

M>'>!c6-0S!6=F!h>!MF478E!!_1;4>!V/D>!D59!O$%%%R!"&^$$k!

?>!(838,!6=F!Q>!V6=F6--E!NH:>!_1;4>!B570!O"***R!a^^>!

A&B! V>!c3H=!et al.E!LM'N?&E!CERN-DD/EE/!84-1!OV/D,4/F!$%ZbR>!

AaB! L>!c6F1+63!et al.>!N60H3/!274!O$%bZR!$&bk!!

'>!cH22,=@08=!et al.E!'9>!h>!248!O$%Z$R!$$b%k!

V>Q>!L8-F/=!et al.E!'9>!h!>479!O$%%bR!%%"k!!

h>!'-:636S!et al.E!_1;4>!Q/00>!B461!O$%%%R!&Zbk!!

(>!)646G,!et al.E!"b01!JTVT!O"**$R!$b$$k!

hH6=!L63:,6#c/--,F8E!93,D60/!:855H=,:60,8=E!@360/2H--;!3/:/,D/F>!

A^B! M>'>!c6-,0SE!h>MF478E!_1;4>!V/D>!D59!O$%%%R!"&^$$k!

)>j>!c63+,:G!et al.,!'9>!h>!Q/00>!482!O$%%bR!Q$%$k!

)>T8H0H!et al.,!'40389630>_1;4>!11!O$%%%R!a"%k!

)>T8H0H!et al.,!"b01!JTVT!O"**$R>!

A[B! _>!)6-60,E!et al.E!NH:->_1;4>_38:>)H99->!81!O"***R!&b>!

AbB! I>!T18H0G8E!L>!Q656==6!6=F!'>!(6-,=,=/E!J=0>!h>!(8F/3=!_1;4>!A17!O"**"R!$Z$b>!

AZB! I>!T18H0G8E!NH:->!_1;4>!B!O_38:>!)H99->R!113 O"**"R!$b*>!

A%B!! l>!e841,5H36!et al.E!_1;4>!V/D>!Q/00>!75!O$%%^R!&b%"k!!

(>!Y82!et al>E!'9>!h>!467!O$%%[R!&&k!

Y>!(604H=6@6!et al.E!_1;4>!V/D>!Q/00>!81!O$%%ZR!a*^"k!

)>!X3,08!et al.E!_1;4>!V/D>!Q/00>!84!O"***R!$*bZk!!

h>j>!(,0:1/--!et al>E!_1;4>!V/D>!Q/00>!76!O$%%[R!&*^bk!!

(>!c8/S,8!et al.E!'9>!h>!487!O$%%bR!a$^k!!

(>!c8/S,8!et al.E!'9>!h>!561!O"**$R!bZbk!

h>!'-:636S!et al.E!_1;4>!V/9>!366/6!O"**"R!&&$>!

A$*B! V>!c600,408=!et al.E!'40389630>_1;4>!13!O"***R!^$>!

A$$B! h>L>!'4.H3;!et al.,!_1;4>!V/D>!Q/00>!18E!"!O$%[bR![^k!

! h>L>!'4.H3;!et al.,!_1;4>!V/D>!Q/00>!19E!$^!O$%[bR!Z[%k!

! C>!c/:G/3!et al.,!_1;4>!V/D>!Q/00>!21E!"$!O$%[ZR!$^*ak!

! Y>!'-D/=4-/./=!et al.,!_1;4>!V/D>!Q/00>!27E!$&!O$%b$R!ZZZ>!!

Page 242: 2004 Ams Nim Paper Draft

AMS-02/Physics

!"#"$*!

A$"B! L>W!c6F+63!6=F!_>(>!XnN/,--E!'FD>!)96:/!3/4>!17/2!O$%%[R!bk!

'>h>!?;-G6E!j>P>!W,/03,:1E!6=F!_>V>!c8./3@E!JMMM!?36=46:0,8=4!NH:>!):,>!44!O$%%bR!"$a*>!!

c>!j,/./-#)8801E!_>Q>!c,/356==!6=F!Y>!(/;/3E!'!o!'!330!O$%%ZR!&Z%>!

A$&B! ! V>!W+;/3E!_>!(/;/3E!'9>!h>!322!O$%ZbR!%Z$k!

h>h>!M=@/-56==!et al.E!'o'!96!O$%%*R!""&k!

l>M>!l385./-E!(>M>!j,/F/=./:GE!'9>!h>!328!O$%ZZR!%a*k!

)>_>!)+83F;!et al.E!'9>!h>!349!O$%%*R!["^k!

'>j>!)038=@!6=F!J>!(84G6-/=G8E!'9h!509!O$%%ZR!"$">!

A$aB! ! j>V>!c,==,4!et al.E!'9>!h>!347!O$%Z%R!%%bk!

_>Y>!P8+-/3!et al.E!'9>!h>!314!O$%ZbR!b&%k!!

(>!J:1,5H36!et al.E!NH8D8!T,5/=08!106A!O$%%&R!Za&k!

_>!(H--/3!et al.E!O"**&R!63\,DK=H:-#/<]*&*"*"^k!!

_>c>!_3,:/!et al.E!_1;4>!V/D>!D18!O$%bZR!$&Z"k!

?>!)6,08!et al.E!_1;4>!V/D>!Q/00>!65!O$%%*R!"*%ak!!

M>l>!)1,3G!6=F!_>c>!_3,:/E!'9>!h>!220!O$%bZR!b$%k!

W6D,F!_>!'=F/348=!et al.E!O"**"R!63\,DK64038#91]*"*^*Z%>!

A$^B! ! _>Y>!P8+-/3!et al.E!'9>!h>!314!O$%ZbR!b&%k!!

h>!(6F4/=E!_1;4>!V/D>!Q/00>!87!O"**$R!$b"k!

h>!)6=F+/,44!h>!_1;4>!L!30!O"**aR!^$!

A$[B! ! I>!T18H0G8E!"Z01!JTVT!4!O"**&R!$b[^>!

A$bB! ! j>V>!c,==4!et al.E!"[01!JTVT!3!O$%%%R!%k!

h>h>!T8==/--E!$%%ZE!'9>!h>!501!O$%%ZR!Q^%k!

L>'>!F/!N8-28!et al.E!"b01!JTVT!5!O"**$R!$[^%k!

?>!Y654!et al.E!"b01!JTVT!5!O"**$R!$[^^k!

'>!QHG64,6G!et al.E!"[01!JTVT!3!O$%%%R!a$k!

(>M>!j,/F/=./:GE!$%01!JTVT!2!O$%Z^R!Za>!

!

Page 243: 2004 Ams Nim Paper Draft

!

Conclusion

'()#*"! ,4! 01/! 2,340! 93/:,4,8=! 9630,:-/! 91;4,:4! /<9/3,5/=0! 8=! 01/! 496:/! 4060,8=>! ! j,01! ,04!

6::/906=:/E!3/48-H0,8=!6=F!6.,-,0;!08!40HF;!F,22/3/=0!9630,:-/4!6=F!=H:-/,!8D/3!&!08!^!;/634!82!F606!06G,=@E!,0!

938D,F/4!6=!899830H=,0;!08!6::H360/-;!/<9-83/!=/+!3/@,8=4!82!91;4,:4>!!!

Acknowledgements

?1/! :8=403H:0,8=! 82! '()#*"! ,4! 6=! H=F/306G,=@! 82! 56=;! ,=F,D,FH6-4! 6=F! 83@6=,S60,8=4>! ! ?1/!

4H99830! 82! N')'! 6=F! 01/! C>)>! W/90>! 82! M=/3@;! 164! .//=! D,06-! ,=! 01/! ,=:/90,8=E! F/D/-895/=0! 6=F!

26.3,:60,8=!82!01/!/<9/3,5/=0>!!?1/!,=0/3/40!6=F!4H99830!82!W6=,/-!)>!L8-F,=E!2835/3!N')'!'F5,=,4036083E!

'>!eH>!VH5;6=04/DE!1/6F!82! 01/!P/F/36-!'@/=:;! 283!'085,:!M=/3@;E!VH44,6E!\H!LH6=1H6E!(,=,40/3!82!

):,/=:/! 6=F! ?/:1=8-8@;E! T1,=6E! 6=F! hm3@! P/H40/-#cp/:1-E! MH389/6=! )96:/! '@/=:;! ,4! @360/2H--;!

6:G=8+-/F@/F>! !?1/! F/F,:60,8=! 82!W3>! h81=!XqP6--8=E!W3>!V8.,=!)0622,=E!W3>!'>!c;8=#j6@=/3! 6=F!W3>!

_>l>!j,--,654! 82! C>)>! WXME! 8H3!(,44,8=!(6=6@/5/=0! 0/65E! W3>! W8H@-64! _>! c-6=:163FE!(3>!(63G! h>!

),40,--,!6=F!(3>!h65/4!V>!c60/4E!N')'E!(3>!l/==/01!c8--+/@!6=F!(3>!?>!(630,=E!Q8:G1//F#(630,=E!01/!

4H99830! 82! 01/! 496:/! 6@/=:,/4! 2385!L/356=;! OWQVR$E! J06-;! O')JRE! P36=:/! OTNM)RE! )96,=! OTW?JR! 6=F!

T1,=6!OT'Q?R!6=F!01/!4H99830!82!T)J)?E!?6,+6=E!16D/!56F/!01/!:8=403H:0,8=!9844,.-/>!

?1/!4H99830!82!L)J#W635406F0E!9630,:H-63-;!82!W3>!V/,=163F!),58=!56F/!,0!9844,.-/!283!H4!08!0/40!

/-/:038=,:4! :8598=/=04! 283! 36F,60,8=!/22/:04>! !?1/! 4H99830!M)'E! ,=:-HF,=@!(630,=!i/--E! h/6=! h6563!6=F!

j8-2@6=@!)H99/3E!+,--!/=6.-/!01/!8D/36--!01/356-!D6:HH5!0/40!60!M)?MT>!!!

?1/! 4H99830! 82! JNPNE! J06-;E! JN"_&E!V/@,8=!V1r=/#'-9/4! 6=F!Y6H0/!)6D8,/E! P36=:/E!TJM('?!

6=F!TJTe?E!)96,=E!QJ_E!_830H@6-E!TYM_E!l83/6E!01/!T1,=/4/!':6F/5;!82!):,/=:/4E!01/!N60,8=6-!N60H36-!

):,/=:/!P8H=F60,8=!6=F!01/!(,=,403;!82!):,/=:/!6=F!?/:1=8-8@;!82!T1,=6E!':6F/5,6!),=,:6E!?6,+6=E!01/!

C>)>!N)PE!(>J>?>E!M?Y#i)3,:1E! 01/!C=,D/34,0;!82!L/=/D6E!N60,8=6-!T/=036-!C=,D/34,0;E!N60,8=6-!)96:/!

_38@365!X22,:/E!N60,8=6-!T16,8!?H=@!C=,D/34,0;!6=F!N60,8=6-!T1/=@!lH=@!C=,D/34,0;E!?6,+6=E!(84:8+!

)060/!C=,D/34,0;E!)8H01/640!C=,D/34,0;E!N6=7,=@E!)16=@16,!h,68!?8=@!C=,D/34,0;E!)H=!e60#4/=!C=,D/34,0;E!

LH6=@S18HE!)16=F8=@!C=,D/34,0;E!h,=6=E!Vj?Y#'6:1/=E!01/!C=,D/34,0;!82!?H3GH!6=F!01/!C=,D/34,0;!82!

?/:1=8-8@;!82!Y/-4,=G,E!,4!@360/2H--;!6:G=8+-/F@/F>!!

j/!63/!6-48!@360/2H-!283!01/!4038=@!4H99830!6=F!,=0/3/40!418+=!2385!01/!93,D60/!4/:083E!,=:-HF,=@!

W3>!M>!M00-,=@/3E!Q,=F/E!W3>!V>!Y/3S8@E!JQlE!W3/4F/=E!(3>!h>!V844E!(3>!)>!(,-+63F!6=F!(3>!)>!Y633,48=!82!

)TQE! TH-165E! ClE! (3>! (>! (8-,=6E! TL)E! (,-6=E! (3>! P>! _/038=,E! T'MNE! I,63/@@,8E! (3>! '>! _846F6E!

TVJ)'!O'403,H5RE!(6F3,FE!J=@>!'>!_8=0/00,E!Lo'!M=@,=//3,=@E!J06-;E!W3>!M>'>!j/3=/3!6=F!W3>!h>!l3,/@/3E!

J)'?MTE!'6:1/=E!6=F!W3>!Y>!c,/3,E!c,/3,!M=@,=///3,=@E!)+,0S/3-6=F>!

j/!016=G!_382/44834!'>!W/!VH7H-6E!h>!M--,4E!'>!LH01E!Q>!(6,6=,E!283!56=;!,=0/3/40,=@!F,4:H44,8=4!

6=F!4H99830>!

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!$!J=:-HF,=@!4H99830!H=F/3!$li!^*!**%%*"!a>!

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A/Acronyms, Abbreviations!

! '#$

Appendix A: Acronyms and Abbreviations

'! '59/3/E!O,=!:85.,=60,8=R!8=/!82!6!4/0!82!3/FH=F6=0!/-/5/=04!

'')! '()!'=0,5600/3!),5H-6083!

'Tc)_! J))!)#c6=F!3/:/,D/3!

'TT! '=0,!T8,=:,F/=:/!T8H=0/34!

'TX_! '()!O83!'4038=6H0E!F/93/:,60/FR!T3/+!X9/360,8=4!_840!

'WT! '=6-8@!08!W,@,06-!T8=D/30/3!

'J)! '=0,5600/3!J=D/40,@60,8=!);40/5!

'()! '-916!(6@=/0,:!)9/:0385/0/3!

'()#*$! '()!/=@,=//3,=@!2-,@10!8=!01/!496:/!41H00-/!

'()#*"! '()!5,44,8=!8=!01/!J))!

'_TC! '44/5.-;!_8+/3!o!T8=038-!C=,0!

'_)! 'H08560/F!_6;-86F!)+,0:1!

')JT! '99-,:60,8=!)9/:,2,:!J=0/@360/F!T,3:H,0!

')?! '5,:6!)063!?36:G/3!

')?M! '5,:6!)063!?36:G/3!M-/:038=,:4!.863F!

')?M! ')?!M-/:038=,:4!

')?_! '5,:6!)063!?36:G/3!_8+/3!.863F!

'C\! 'H<,-,63;!

'jL! '5/3,:6=!j,3/!L6H@/!

c!! 485/0,5/4!c;0/E!485/0,5/4!c,0!

cT)! c/301,=@!TH/!);40/5E!6-48!McT)!

cXQ! c/@,==,=@!82!Q,2/!

T! T3;856@=/0!O,=!:85.,=60,8=RE!T8-F!O,=!:85.,=60,8=R!

T!o!W! T8556=F4!6=F!W606!

T'c! T3;856@=/0!'D,8=,:4!c8<!

T'MN! T8403HS,8=,!'9963/::1,60H3/!M-/0038=,:1/!NH:-/63,!E!)>9>'>!!

T'N! T8=038--/3!'3/6!N/0+83G!

TT! T3;8:88-/3!O,=!:85.,=60,8=R!

TTc_T! TTMc!c6:G9-6=/E!T8=038-!

TTc__! TTMc!c6:G9-6=/E!_8+/3!

TTc?! TT!&W!Y6--!_38./!6=F!_?)!3/6F8H0!

TTWT! TT!WT#WT!T8=D/30/3!.863F!

TTMc! T3;8:88-/3!M-/:038=,:4!c8<!

TTJP! TT!J=0/326:/!c863F!

TT(W(! T8556=F!o!T8=038-!(W(!

TT(X! TT!(8=,083!o!X4:,--6083!

TT_'! TT!_8+/3!'59-,2,/3!

TT)! T3;856@=/0!T163@,=@!);40/5!

TT)T! T3;856@=/0!T8=038--/3!6=F!),@=6-!T8=F,0,8=/3!!

TWW! T3;856@=/0!WH59!W,8F/4!

TWWT! T8556=F!W,403,.H083E!W606!T8=:/=036083!

TW_! T8558=!W,@,06-!_630!

TMVN! MH389/6=!T/=0/3!283!NH:-/63!V/4/63:1!

TL)! T63-8!L6D6SS,!)96:/!)9'E!J#(,-6=8!

TL)M! T;38@/=,:!L38H=F!)H99830!MUH,95/=0!

TQE!T>Q>! T8=2,F/=:/!Q,5,0!

T_! T163@/!_63,0;!

:_TJ! T8596:0!_TJ!.H4!283560!

TVJ)'! T859H06F8364E!V/F/4!/!J=@/=,/3,6E!)>'>!

T)_! T3;856@/=0!)/-2!_380/:0,8=!:,3:H,04!

TIc! T3;856@/=0!I6-D/!c8<!

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!'#"!

W!! F/H0/38=!

W'T! W,@,06-!08!'=6-8@!T8=D/30/3!

W'g! W606!':UH,4,0,8=!

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WT#WT! WT!08!WT!:8=D/30/3!

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FM]F\! M=/3@;!-844!+1/=!036D/34,=@!5600/3!

WM)e! W/H04:1/4!M-/G038=/=#);=:138038=!

W)_! W,@,06-!),@=6-!_38:/4483!

W?)! W,@,06-!?/59/360H3/!)/=483!O/>@>!W)$Z)"*R!

M! MT'Q!O,=!:85.,=60,8=R!

M#T360/! MT'Q!T360/!

McT)! M<0/3=6-!c/301,=@!TH/!);40/5!

Mc_! M#T360/!c6:G9-6=/!

MT'Q! M-/:03856@=/0,:!T6-83,5/0/3!

MWV"! MT'Q!W606!V/FH:0,8=!.863F!O:8=06,=4!0+8!MWVR!

MYI! MT'Q!YI!c3,:G!

M(! M=@,=//3,=@!(8F/-!

M(T! M-/:03856@=/0,:!T85960,.,-,0;!

M(J! M-/:03856@=/0,:!J=0/32/3/=:/!

MXQ! M=F!82!Q,2/!

M_W! MT'Q!_8+/3!W,403,.H0,8=!.8<!

M_)PM! MT'Q!_8+/3!)H99-;!283!P38=0!M=F!.863F!

M)'! MH389/6=!)96:/!'@/=:;!

M)?MT! M)'!MH389/6=!)96:/!V/4/63:1!6=F!?/:1=8-8@;!T/=03/!

M?VL! MT'Q!?3,@@/3!.863F!

MI'! M<036D/1,:H-63!':0,D,0;!

P]X! P,./3!890,:!

PM! P38=0!M=F!

PJPX! P,340!J=E!P,340!8H0!

P(! P-,@10!(8F/-!

P)! P-,@10!)963/!

L! L6H44!O*>$!5?R!

@! %>Z!5]4]4E!@365!

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L_)M! J=0/326:/!283!L_)!O?894063!&***W!sR!

L)T! L38H=F!)H99830!T859H0/34!

L)M! L38H=F!)H99830!MUH,95/=0!

L)PT! L8FF63F!)96:/!P-,@10!T/=0/3!

L)J! L/4:1/--4:1620!2p3!):1+/3,8=/=2834:1H=@!

Y! Y80!O,=!:85.,=60,8=R!

YTXV! YVWQ!T855H=,:60,8=!XH06@/!V/:83F/3!

YX)T! YH=0D,--/!X9/360,8=4!6=F!):,/=:/!T/=0/3!

YVWQ! Y,@1!V60/!W606!Q,=G!

YVP(! YVWQ!P365/!(H-0,9-/</3!

YV(! YVWQ!(8F/5!

YI! Y,@1!I8-06@/!

J! TH33/=0!

JTW! J=0/326:/!T8=038-!W8:H5/=0!

JP_!'! J=0/326:/!_6=/-!'!

J)_V! J))!)06=F63F!_6;-86F!V6:G!

J))! J=0/3=60,8=6-!)96:/!)060,8=!

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! '#&

JI?! J=0/326:/!I/3,2,:60,8=!?/40!

h! W'g!83!L-8.6-!O,=!:85.,=60,8=R!

h#T360/! (6,=!T859H0/3!6=F!J=0/326:/!T360/!

hc_! h#T360/!c6:G9-6=/!

hcC! h(WT!"t$Lc!(/583;!cH22/3!

hYJP! V/FH=F!YVWQ!OJ))RuhPX(!f!4,=@-/!V)a""O)?)Ruha""!J=0/326:/4!

hJ(#'()jo$^^&! h(WT!J=0/326:/!08!'()j,3/!o!QVWQ!!D,6!hQJP!OJ))R!o!$^^&!O)?)R!

hJ(#T'N! h(WT!J=0/326:/!08!T'N!

hJ(#YVWQ]a""! h(WT!J=0/326:/!08!YVWQ!OJ))R!83!V)a""!O)?)R!D,6!hYJP!

hJNP! W'g!J=0/35/F,60/!N8F/E!P38=0!M=F!

hJNh! W'g!J=0/35/F,60/!N8F/!

hJNV! W'g!J=0/35/F,60/!N8F/E!VJTY!

hQJP! V/FH=F6=0!QVWQ!O$^^&Ruh$^^&!J=0/326:/4!

hQI$! Q/D/-#$!03,@@/3!938:/4483!

h(WT! (6,=!W'g!T859H0/3!

h_c_! h_W!.6:G9-6=/!

h_W! h#!6=F!h?#T360/!_8+/3!W,403,.H0,8=!.8<!

h_JP! WT#WT!o!(oT!283!hYJP!o!hQJP!

h_h?! WT#WT!o!(oT!283!h?!!

h_(W! WT#WT!o!(oT!283!"!h(WTq4!

h_)T! WT#WT!o!(oT!283!C)T(E!h_W!,=0/3=6-4!

h)cT! h(WT!),=@-/!c863F!T859H0/3!

h)T! h81=48=!)96:/!T/=0/3!

h?#T360/! ?3,@@/3!o!W'g!T360/!

h?c_! h?#T360/!c6:G9-6=/!

h?c\! 2640!03,@@/3!4,@=6-!26=!,=]8H0!o!-8@,:>!

h?_W! ?3,@@/3!_8+/3!W,403,.H083!O4H993/44/FR!

l!! F/@3//4!l/-D,=!

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Gj! $***!j600!

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QT?Q! Q64/3!'-,@=5/=0!:8=038-!.863F!O+64!Q'TR!

QWWV! Q64/3!'-,@=5/=0!F3,D/3!.863F4!O+64!Q'WR!

Q(! Q8:G1//F#(630,=!

QY/! Q,UH,F!1/-,H5!

QY_! Q889/F!Y/60!_,9/!

QN! Q,UH,F!=,038@/=!

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(! (644E!(8=,083!o!T8=038-!O,=!:85.,=60,8=R!

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(W(! (H-0,9-/</3]W/5H-,09-/</3!

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(Q_! (8.,-/!Q6H=:1!_-602835!

((X! N')'!'()!(,44,8=!(6=6@/5/=0!X22,:/!

(X)PM?! (/06-!X<,F/!8=!),-,:8=!P,/-F!M22/:0!?36=4,4083!

(_W! (8=,083!o!T8=038-!_8+/3!W,403,.H083!

()PT! (63416--!)96:/!P-,@10!T/=0/3!

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A/Acronyms, Abbreviations!

!'#a!

N')'! N60,8=6-!'/38=6H0,:4!6=F!)96:/!'@/=:;!

NcQ! N/H036-!cH8;6=:;!Q6.!

_! 585/=0H5E!93/44H3/E!938.6.,-,0;E!O,=!:85.,=60,8=R!_8+/3E!_830E!_3,563;!

9! 93808=E!585/=0H5!

_')! _6;-86F!'006:1!);40/5!

_T'! _3,=0/F!T,3:H,0!'44/5.-;!

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_Wc! _8+/3!W,403,.H0,8=!c8<!OF,426D83/FR!v!4//!_W)!!

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_Q(W(! _6;-86F!(W(!

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_ILP! _8+/3!6=F!I,F/8!L3699-/!P,<0H3/!

g! :163@/!

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A/Acronyms, Abbreviations!

! '#^

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)_XM! )06=F63F!_6;-86F!XH02,00,=@!MUH,95/=0!

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?! ?/4-6E!),-,:8=!?36:G/3!O,=!:85.,=60,8=R!

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A/Acronyms, Abbreviations!

!'#[!

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B/Bibliography

! c#$

Appendix B: AMS Principal Publications

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C/Collaborators

!

! T#$

Appendix C: Collaborating Institutes and Universities

Institute Location Contact

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C/Collaborators!

!T#"!

Institute Location Contact

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