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SESAME Synchrotron Light for Experimental Science and Applications in the Middle East JSPS Asien Science Seminar Synchrotron Radiation Science Dieter Einfeld Amman, October 2002

JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

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Page 1: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

SESAMESynchrotron Light for Experimental Science and Applications in the Middle East

JSPS Asien Science Seminar

Synchrotron Radiation ScienceDieter Einfeld

Amman, October 2002

Page 2: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

IntroductionBased on the workshops held in the Middle East Region and other activities of the SESAME Scientific Committee, the scientific program for SESAME includes:

Structural molecular biology Molecular environnemental scienceSurface and interface scienceMicro mechanical devicesX-ray imagingArchaeological microanalysisMaterial characterizationMedical applications

Most of these applications require hard x-rays up to 20 keV photons.

Page 3: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Characterization of Synchrotron Radiation

S

Y

X

As = Cross section of electron beam

X-ray‘s

X-ray‘s

Φ

ψ

Flux = Photons / ( s • BW)

Brilliance = Flux / ( As • ∆Φ •∇ψ) , [ Photons / ( s • mm2 • mrad2 • BW )]

Fluxdensity = Flux / As , [ Photons / (s • mm2 • BW)]

∆φ / ∆ψ = Opening angle in vert. / hor. direction

Page 4: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Performance of a Light Source

The performance of a synchrotron light source is given by:

the brilliance of the emitted radiation

the overall length of the straight sections

the emitted photon spectrum

The brilliance:The brilliance is proportional to the photon flux per area of the source size, and opening angle of the radiation. Both factors are proportional to the emittance of the stored electron beam.

To increase the brilliance further more one introduces wigglers and undulators to enlarge the number of source points.

Page 5: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Performance of a Light Source

Length of the straight sections:According to the attraction of the synchrotron radiation, a light source should provide the radiation simultaneously to a lot of users. Hence the performance of a synchrotron light source is proportional to the number of useable long straight sections.

The photon spectrum:The different users are asking for a special spectrum range. The highest photon energy of the spectrum from the bending magnet, the wiggler and the undulator is proportional to the square of the energy of the stored electrons. So, the performance of the machine should also proportional to the energy.

The following parameters of the machine determine the performance of a synchrotron light source:

the emittance

the overall length of the straight sections

the energy

Page 6: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

History of SESAME

Idea to upgrade BESSY I (1997)

Proposal for SESAME to UNESCO DG (1999)

Establishment of Interim Council

Setting up of Advisory Committees (international)

Green Book (Technical Proposal) (1999)

Site Decision Al-Balqa Applied Universit

Training Programme initiated (Oct. 2000)

Financing of BESSY I dismantling (Aug 2000)

Appointment of Technical Director (Sept. 2001)

New Advisory Committees (from region)(Dec. 2001)

Shipping of BESSY I components (May 2002

Page 7: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

History of SESAMEGreen Book Design:

Photon energies of 20 KeV are required

7.5 Tesla super conducting wiggler is available

To reach 20 keV photons, the energy has to be increased to 1 GeV

The bending magnets have to be modified ( from 1.5 to 1.87 Tesla)

All magnets (quadrupoles and sextupoles) from BESSY I should be used

The number of straight sections have to be increased

Solution:New arrangement of magnets ( Circumference = 100.4 m )

Energy = 1 GeV, emittance = 50 – 100 nm rad,

Number of straight sections = 6 ( only 3 for wigglers )

Conclusion:The design of the „Green Book“ has to make a lot of compromises. With the result, that the specifications can not compete with other synchrotron light sources.

New design, White Book

Page 8: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

History of SESAME

White Book Design:Design of building based upon ANKA

Building: ANKA plus annexes

Lengths of beam lines around 30 meter

Maximum circumference of the storage ring is 126 meter

The energy was fixed to 2 GeV

New arrangements of magnets (TME – optic)

16 straight sections ( 8 long & 8 small )

Emittance is around 17 nmrad

Radiation spectrum from bendings goes up to 12 keV

Radiation spectrum from wiggler goes up to 24 keV

Repetition frequency of booster will changed to 1 Hz

Page 9: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Bending Flux

1E+12

1E+13

1E+14

0.001 0.01 0.1 1 10 100

Energy [keV]

Phot

ons

/ sec

ond

Wh.-Book Gr.-Book

Flux of the synchrotron radiation from the bending magnets: Version SES_1_1: Green book, 1GeV, 1.87 Tesla, 400 mA; version SES_4_2: 2GeV, 1.35 Tesla, 400 mA

Radiation CharacteristicsMachine

Page 10: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Wiggler Flux

1E+12

1E+13

1E+14

1E+15

1E+16

0.01 0.1 1 10 100Photon Energy [keV]

Phot

./ s

GR.-Book Wh.-Book

Flux of the synchrotron radiation from the wiggler for the versions: SES_1_2 and SES_4_1.

Radiation CharacteristicsMachine

Page 11: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Bending Brilliance

1E+12

1E+13

1E+14

1E+15

0.01 0.1 1 10 100Photon Energy [keV

Phot

ons/

s*m

m^2

*mra

d^2*

Bw

Gr.-Book Wh.-Book

Brilliance of the synchrotron radiation from the bending magnets for the versions SES_1_2 and SES_4_1

Radiation CharacteristicsMachine

Page 12: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Wiggler Brilliance

1E+13

1E+14

1E+15

1E+16

1E+17

0.01 0.1 1 10 100Photon Energy [keV]

Phot

./ s*

mm

^2*0

.1B

WGr.-Book Wh.-Book

Brilliance of synchrotron radiation from the wigglers of the versions SES_1_2 and version SES_4_1

Radiation CharacteristicsMachine

Page 13: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Bending Brilliance

1E+11

1E+12

1E+13

1E+14

1E+15

0.01 0.1 1 10 100Photon Energy [keV]

Phot

/s*m

m^2

*mra

d^2*

0.1B

WGr.-Book Wh.-Book

Brilliance of the synchrotron radiation from the bending magnets for the versions SES_1_2, SES_3_2, SES_2_2 and SES_4_2.

Radiation Characteristics

Brilliance of the synchrotron radiation from the bending magnets for the versions SES_1_2 and SES_4_2

Machine

Page 14: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Wiggler Brilliance

1E+13

1E+14

1E+15

1E+16

1E+17

1E+18

0.01 0.1 1 10 100Photon Energy [keV]

Phot

./ s*

mm̂

2*0.

1BWGr.-Book Wh.-Book

Brilliance of the synchrotron radiation from the wigglers forthe versions SES_1_2 and SES_4_2

tics Radiation CharacteristicsMachine

Page 15: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Radiation Characteristics

Opening Angle of Synchrotron Radiation

0

0.2

0.4

0.6

0.8

1

0.1 1 10 100Photon Energy ( KeV )

Ope

ning

Ang

le (m

rad)

Page 16: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

SESAMESynchrotron Radiation Facility

E= 2.0 Gev ε= 17.3 nm.rad C= 126 m

Machine

Page 17: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Machine

Machinefunctions

0

2

4

6

8

10

12

14

16

18

20

0 2 4 6 8 10 12 14Length (m)

Mac

hine

func

tions

(m/ra

d)

Magnets BETA(x) BETA(y) DISP(x)

Page 18: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Optical functions of SESAME lattice, the green line represents dispersion. Horizontal and vertical correctors are represented in red and blue.

Machine am Optics

Beam Cross sections

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0 5 10 15

Length (m)

Cros

s se

ctio

n (m

m)

Sigma(x,Betax) Sigma(y) Sigma(x) Lattice

Page 19: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Machine

Beam Divergencies

00.10.20.30.40.5

0 2 4 6 8 10 12 14

Length (m)

Dive

rgen

cy (m

rad)

Lattice X-Pri_Beta Y-Prime X-Prime

Page 20: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

E (Gev) 2C (m) 119.51

εx (nm.rad) 17.3Qx , Qz 7.272, 5.216ξx , ξz -13.608, -14.889

βx , βz , ηx(m)

12.6, 1.14, 0.52 (in 8 Sec.)8, 2.47, 0.4 (in the others)

# BMs 16

Bo(T) , k 1.35, 8.327 (k=-0.341)

# Quads 48 (3 families)

# Sext. 64 (4 families)# Str.

Sections 16 (8 x 3 m + 8 x 3.12 m)

Parameters Parameters of the of the SESAME SESAME Storage Storage RingRing

800 MeV Booster Synchrotron

800 MeV Booster Synchrotron

Machine

Page 21: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

One Unit Cell

Vacuum System

Machine

Page 22: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Dipole #1

Dipole #2

MachineB1

B2 B1

Page 23: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Quadrupole

Sextupole

One unit Cell

Vacuum pump

Dipole

Machine

Page 24: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Arrangement of Magnets adjacent to Dipole Number One

Machine

Page 25: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Dipole Number Two

Machine

Page 26: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Long Straight Section of the SESAME Storage Ring

Machine

Page 27: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Short Straight Section of the SESAME Storage Ring

Machine

Page 28: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

A possible arrangement of the beam lines within the experimental hall

A possible arrangement of the beam lines within the experimental hall

Page 29: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Bea

m L

ines

and

ther

e L

engt

hs

Page 30: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Arrangement of the Control

Hutches

Page 31: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Front Ends and Beam Lines

Page 32: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Front End of the Beam Lines at ANKA

Page 33: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

LIGA-I Beam Line at ANKA

Page 34: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

LIGA-II Beam Line at ANKA

Page 35: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

LIGA-III Beam Line at ANKA

Page 36: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Diffraction Beam Line at ANKA

Page 37: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Fluorescence and Topography Beam Line at ANKA

Page 38: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Protein Crystallography Beam Line at ANKA

Page 39: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

X-Ray Absorption Beam Line at ANKA

Page 40: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Infrared Beam Line at ANKA

Page 41: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

SESAMESynchrotron Radiation Facility

E= 2.0 Gev ε= 17.3 nm.rad C= 126 m

Page 42: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

General View of the Building and the college

Page 43: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

General layout of the SESAME Site

Page 44: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

North Elevation

South Elevation

Page 45: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

West Elevation

East Elevation

Page 46: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Technical Building

Page 47: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Space within the Ground Floor

Num Description (Ground Floor) Area (m2)

1 Experimental hall 4473.512 Large laboratories (12*52,5) 630.71 Small laboratory 25.61 Mechanical workshop 83.21 Electrical workshop 56.51 Multipurpose hall 25.41 Main entrance 168.43 Staircase ( 3*25.7) 77.12 Female / male toilets 109.42 Mechanical & electrical services 54.7

Total: 5704.5

Page 48: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

Num Description Area (m2)

1 Control room 54.41 Maintenance room 34.62 Store rooms 49.01 Seminar room 54.51 Library room 56.23 Meeting rooms 113.62 Service rooms 18.06 Secretary rooms 105.93 Director rooms 104.020 Offices 400.03 Staircases 77.25 Female / male toilets 136.42 R.F. power supply rooms 36.4

2 Service rooms 18.01 Lobby 535.9

Total: 1794.1

Space within the First Floor

Page 49: JSPS Asien Science Seminar Synchrotron Radiation Scienceconference.kek.jp/JASS02/PDF_PPT/5_einfeld.pdf · According to the attraction of the synchrotron radiation, a light source

First floor with the bridge from the control room to the inner side