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International Conference On Cosmic Rays JAIPUR, DECEMBER 2-14, 1963 Under the auspices of The International Union of Pure and Applied Physics and The Department of Atomic Energy, Government of India PROCEEDINGS Edited by R. R. Daniel P. J. Lavakare M. G. K. Menon S. Naranan N. W. Nerurkar Yash Pal B. V. Sreekantan

International Conference OnCosmic Rays · 2008. 7. 15. · of the Coaaic Radiation N. Durgapraaad 17 5-6. Flux and Energy Spectra of Heavy Primary H-lagoda Huolei Meaaured on Polar

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  • International Conference On Cosmic Rays

    JAIPUR, DECEMBER 2-14, 1963

    Under the auspices of

    The International Union of Pure and Applied Physics

    and

    The Department of Atomic Energy, Government of India

    PROCEEDINGS

    Edited by

    R. R. Daniel P. J. Lavakare

    M. G. K. Menon S. Naranan

    N. W. Nerurkar Yash Pal

    B. V. Sreekantan

  • Yolom* §

    contents

    OOSgOSITIOW

    5- 1. Lightp Hsdlum and Heavy Nuclei in the

    Primary Spectrum in 3.965 at Minneapolis

    W»R. Webber

    J. Ormss

    Page

    S

    5-2. A sitter of the Multiply Charged Nucleiof th® Primary Cosmic Equator usingNuclear Emulsions - Part Is Fragmanta-

    tion Parameters in Graphite

    G.D. B&dhvarN. DurgapraaadB.ViJayalakshal

    8

    3- 5. A Study of the Multiply Charged Nuclei G.D, Badhvar

    of the Primary Cosmic Radiation near the N .Durgapraaad

    Geomagnetic Equator using Nuclear Emulsions B. Vljayalakahmim Part lit Chemical Composition of tha

    Primary Cosnio Ray Nuclei of Charge %>, 6.

    IS

    5-4. A Study of Multiply Charged Nuclei oftha PriBAry Coaaic Radiation near the

    Geomagnetic Equator using NuclearEmulsions - Part III* The Light Nuclei

    of the Coaaic Radiation

    N. Durgapraaad 17

    5- 6. Flux and Energy Spectra of Heavy Primary H- lagodaHuolei Meaaured on Polar Orbiting Sata- K. Fukni

    llitea

    24

    8- 6. Study of the Relative Abundance of tha

    Primary Cosmic Ray Nuclei with Z * 26

    0, AlvialJ. Riquelmi

    52

    5- 7. Energy Spectrum of Heavy Nuclei of

    Primary Cosmic Rays fro* simultaneous

    Flights from Texas, USA and Hyderabad,India

    G.D.Budhvar

    S. Bievas

    R.B. Daniel

    N.Durgapraaad

    58

    5- 8. Cosmic Ray Nucleus Component Investi¬

    gation Performed on Soviet Satellites

    and Probes

    V.L. Ginsburg 41

    V.I. LugaoiJetL.A. Rax&renov

    M.I. Fradkin

  • 'Mmm—u

    8- 9. Caaages ia tha Primary Cosaie Bay

    Proton Spectrum la 19§I ®M 19*8?• MayerB. ¥©gt

    49

    S-IQ. The Primary Goaale lay Proton Flux

    over Hyderabad, India

    ¥•£« BhattB.R. ©@ai®JL

    se

    5-11. The Energy- Spectrum of Primary Cosmic

    Bay Protons of Energy 8-iS 6»V from

    eimultameoaa Flights aad« from Texaa

    USA and Hyderabad, India

    BJUD&niel 60

    N .SraanivauBia*

    5*12. Tha Flux of Primary Cosaie Ray Daute-

    rons at a Gaosagnatie Latitude ofS.H. GaaguX± 68H.Kameewara», Rao

    M«S. Svaml

    9*18. Low Energy Protons, Deuterium aad

    Alpha Particles in the PrimarySpectrum in 1968 at Ft. Churchill

    and Minneapolis

    V.B. Vabb*arJ. Oraaa

    69

    5-14. Cosaie Ray Intensity at Thule,Greenland and its Relation to Data

    from Mariner II

    H.7. Nefaar 76H.R.Anderaon

    KBKKjBUCSLm^m^^BMmm

    5-15. Iaotoplc Abundance of Carbon Nuclei in

    Primary Coaaic Rays

    H. Haaegavam.H. Aisu

    K. Ito

    88

    5-16. On the Isotopic Composition of HydrogenNuclei in Low Energy Primary Coaaic

    Radiation

    H. Hasegatraa,S. Nakagawaa,S. Tamai

    86

    5-17. Iaotoplc Abundance of Helium Nuclei inPrimary Coaaic Radiation

    H. Aisu 90

    5-18. The Iaotoplc Composition and tha EnergyHelium Nuclei in Primary Cosmic Radiation

    M.V.K.Appax BaoC. Dahaney-smkeMJ. Kaplcaaa.PJT. Lavakffitre

    98

  • 5-19, The Helium Isotopes in th® PrimaryCosmic Radiation

    BJiildebramd

    F.W. O'DellM.M. ShapiroR. SilborhergB. Stillmr

    101

    5-20. An Attempt to Determine tha laotopieComposition of High Energy HeliumNuclei in th® Primary Cosmic Radiation

    V *K .BalaaubraaanyanS.7. DaaleG.S. Gokhale

    M.G.S. Manon

    S.K. Roy

    5-21. Determination of Carbon Isotopes inthe Primary Cosmic Rays

    G. Alvial 116

    5*22. A Measurement of Low Energy Coaaio RayProtons

    K.A. Brunstein 1£0

    ELECTRONS AND PHOTONS

    SSSSI9J I

    5-25. Electrons and Photons in the PrimaryCosmic Rays

    S. Hayaxawa 125

    5-24. The Ratio of Electrons to Positrons

    in the Primary Cosaio Rays

    J.A.Da Shong Jr. 155R.H.Hildebrand

    P. Mayer

    5-25. Some Problema in Connection with

    Galactic Electrons

    N. Lund

    B. SwanenhurgI. TanakaA.H. Vapstra

    165

    5-26. Investigation of Primary Electrons

    at 46° Geomagnetic Latitude

    B. AgrinierT. Koechlin

    B. Parller

    G. Boalla

    G. Degli AntoniC. Dilworth

    L. Scare!

    G. Sironi

    167

  • SESSION II

    5»270 Gaaaa and x-Radiation Connected with

    the Galactic and MstagalacticCosmic Rays

    ?.L. Ginsburg

    S.I.Syrovat@ky177

    5-28. Cosmic Gamma Ray Results from Explor¬er II

    tf«L. Kr&uahstar

    G.W. ClarkM. AgaglnoG. Garmir®H« Helmken

    P. Higbi®

    184

    5-29, Investigation of Primary Gamma Rays E.M, HafnorJ.G. Duthla

    MJ\ KaplonG. Share

    190

    5-50. 100 Channels, 0.1 to 2 M»V Gamaa-

    Speetroaater of the Earth's Atmos¬phere between 0 and 160 km

    D* Boolet

    A. Duoros

    J. Labeyrie)R. Rocohia

    194

    5-51. Gaaaa-Ray Spectrometer for Balloon

    FlightsD. KohnK. PinkauG. Wibberrena

    208

    5-52. x-Ray Production in SupernovaRemnants

    G. ClarkM. Oda

    206

    5-55. Possible Local Sources of Galactic

    x-RaysS. HayakavaM. Matsaukav

    215

    General Disucsslon on Composition 219

  • ORIGIN

    SESSION I

    5-54, The Production of Cosmic Rays in ViolentEvents in Galaxies

    G. Burbidge 229

    5-55, The Origin of Cosmic Rays V.L. GinaburgS.I.Syrovatsky

    501

    SESSION H

    5-56. Cosmic Rays from Large Supernovas S.A. ColgateR.H. White

    555

    5-57. Cosmic Ray Energy Spectrum and High-Energy Particles in Supernova

    H. Sato 560

    5-58. Possible Anisotropy of Coaaic Rayswith Respect to a Spiral Arm

    S. HayakawaH. ObayashiS. Sakakibara

    564

    5-59. On the Configuration of Relativistic

    Particles Generated by a Supernovain the Galactic Arm and an Inter¬

    pretation of the Radio Spur

    M. Oda

    H. Kasegava

    570

    SESSION III

    5-40. Cosmic Ray Equilibrium W .L .Kraushaar 579

    5-41• Results of Calculation of EnergySpectrum of Galactic Cosmic Rays

    A.N.CharkhchyanT .N .Charakhcbyan

    584

    5-42. Transformation in the Composition of

    the Galactic Coemic Radiation

    during its Traversal in Space

    G.D. Badhwar

    R.R. Daniel

    B.VljayalakabjBi

    590

  • &»4S, Primary Cosmic Radiation of Ultra

    High Energy

    G«B«Kristian0

  • mmL~a

    5»49. Comic Ray Data Derived from IsotopeStudies in Meteorite

    H. Manke 475

    S-60, The Temporal and Spatial Variationin Cosmic Rays

    O.A.3ehaeffer

    R. Davis Jr.

    R.H. Stosnner

    D. Heyaann

    480

    5-51. Solar Surface Nuclear Reactions EX. Fireman 487

    Concluding Remarks B. Peters504

    Author Index509

  • EXTENSIVE AIR SHOWERS

    Scientific Secretaries:

    S. Naranan

    B. K. Chatterjee

    T. Matano

    G. T. MURTHY

    M. V. Srinivasa Rao

  • Volume 4

    ECTEMSIVE AIR SHOWERS

    CONTENTS

    SESSION I

    4- 1, A general account of the various research V, Domingoactivities at Chacaltaya

    Page

    4- 2. Evidence for extensive air showers with

    extremely few penetrating particlesK. SagaI. Escobar

    K. MurakamiV. DomingoY. ToyodaG. Clark

    M. La Polnte

    4- S. The British Universities extensive air

    shower project at Haverah ParkJ.G. ¥ilson

    H.R. Allen

    S.C. LillicraP

    R.J.O. Held

    K.E. rarvor

    27

    4-4. Extensive air shower studies in Australia G.B.A.MoCusker 55

    4- 5. Primary energy spectrum from 6.101to 4.10 ev

    G. Clark

    H. BradtM. La PointeV. DomingoI, EscobarK, MurakamiSo SugaY. ToyodaJ. Hersll

    65

    4— 6.

    17primary cosmic rays of energy 10

    to

    102° evj the energy spectrum andarrival directions.

    J, Linsley 77

    4- 7. Extensive aix showersof cosmic radia¬

    tion

    G.T. lataepinS.I, NikolskyG.B. Khristiansan

    100

  • smm-Bi

    8. Extensive air showers - studies of

    Tokyo group

    T. Mateno

    I, Miura

    M. NaganoH. Oda

    S. Shlbata

    I. Tanaka

    G. Tanahashi

    H. Hasegawa

    129

    4- 9. Extensive air shower studios of th©

    TUR (Bombay) groupB«V. Sreekantan 145

    4-10. Character of air showers at 5,200 aaltitude

    I. Escobar

    V, DomingoK, MurakamiK. SugaY» ToyodaG. Clark

    M. La Pointe

    M» Oda

    H. Bradt

    I. Miura

    M. NaganoS. Shlbata

    G. Tanahashi

    H. Hasegawa

    168

    4-11, A description of a Modified complexinstallation for Investigationof extensive air showers andnew experimental data obtained

    by means of this installation.

    S.N, fornoTG.B. KhristiansenA.M. Abrosisov

    "V.B. AtrashkevichM.F, BeliaevaO.K. Vedeneev

    V,A. DmitrievG.H. Kulikov

    Yu.A, N@«hinV.I. Solovieva

    K.I. Solo¥i®wXu,A. FondaB.A. Khrenov

    175

    4»12. Further data on the photonic exten¬sive air showers

    J, GawinJ, Hibner

    A. ZawadtOd.E. Mass

    ISO

  • SESSION IV

    4-13, Arrival direction of uu-rich airshowers

    Y, Sekido

    S, Sakakibara

    189

    4-14. Studies on the anisotropy of cosmic

    rays with the cosmic ray tele¬

    scopes in .Nagoya

    Y. Sekido

    I. KondoT. MurayaaaY. KsmiyaH. Ueno

    S. Mori

    H. Okuda

    T. Makino

    S. Sakakibafa

    K. Jujimoto

    194

    4-15. On the high energy photons fromlocal sources

    A.E. ChudakovV.L. DadykinV.I. ZatseplnN.M. Keaterova

    190

    4-16. Core structure and properties of

    extensive air showers

    S* MlyakeK. Hinotani

    T® Kaneko

    N. Ito

    205

    4 »17. Development of vertical extensive

    air showers in the upper part

    of the atmosphere

    R«A* Antonov

    Yu.A, Smorodin

    Z.I. Tulinova

    209

    4-18- The altitude variation of air

    showers

    K. Kemata

    K. Murakami

    S. Kawasaki

    214

  • SESSION V

    4-19. Nuclear-active particles in showerswith different number of

    particles

    T,V. Danllova

    S.I. Nikolsky

    £21

    4-201 Studies gn extensive air showers4-2l| (10 ~ 1° ) at mountain alti-4-22J tude (800 g cm2)

    B.K. Chatterje©G.T. MurthyS. Naranan

    B.V, Sreekantan

    M,V, arinlvasa Rao

  • 4-27, Anisotropy of rauon rich extensiveair showers

    T. Matano

    I. MiuraM« NaganoM. Oda

    S. Shibata

    Y. Tanaka

    G. Tanahashi

    H, Hasegawa

    248

    4-28. N-partlcles in extensive air showers T, KamedaY. ToyodaT. Maeda

    254

    4-29. Arrival directions of large extensive B.R. Dennisair showers J.G. Wilson

    258

    4-30, Multiple muon events in air showersat sea leyel

    R.G. BinghamE.W, Kellermann

    261

    §SfflIPJLJI

    4-31. The density spectrum of extensive airshowers at very largd densities

    T. GemesyA. SomogylG. Valas

    267

    4-32. Study of the properties of the pene¬trating component of extensiveair showers at.the depth of200 mwe.

    T.T. Barnaveli

    I.F. BibilashviliG,A, Grubelashvili

    A.K. Javrishvili

    R.E. Kazarov

    R.V. Kuridze

    I.V. Khaldeeva

    273

    4-33* Absorption characteristics of muonsin extensive air showers

    K. Hinotani

    S. MiyakeM.V, Srinivasa Rao

    277

    4-34, The fluctuation of densiby of tnuonain extensive air showers.

    H. HasegawaT. Matano

    I, Miura

    S, Shibata

    284

  • 4-35. Production in the atmosphere of exten- T. Matano 290sive air showers containing very V,S, Narasimhamfew muons

    4-36. Air shower fluctuations J. Lineley'

    295 -

    4-37. Two large air shower experiments C.B.A. McCusker 306H.D. Rathgeberh.M, Winn

    SESSION VII

    GENERAL DISCUSSION 313

    Author Index 321