Study of primary cosmic ray composition from gamma ray families in air shower cores

被引：0
|
作者：
Honda, K
Kawasumi, N
Tsushima, I
Hashimoto, K
Nishida, T
Matano, T
Inoue, N
Ohsawa, A
Tamada, M
Ohmori, N
Martinic, N
Ticona, R
Gironda, N
Osco, F
Aguirre, C
机构：
[1] FUKUI UNIV TECHNOL,DEPT APPL PHYS & CHEM,FUKUI 910,JAPAN
[2] SAITAMA UNIV,FAC SCI,URAWA,SAITAMA 388,JAPAN
[3] UNIV TOKYO,INST COSM RAY RES,TANASHI,TOKYO 188,JAPAN
[4] KINKI UNIV,FAC SCI & TECHNOL,HIGASHIOSAKA,OSAKA 577,JAPAN
[5] KOCHI UNIV,FAC SCI,KOCHI 780,JAPAN
[6] UNIV MAYOR SAN ANDRES,INST INVEST FIS,LA PAZ,BOLIVIA
来源：
NUCLEAR PHYSICS B | 1997年
关键词：
D O I：
暂无
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
We have observed high energy gamma families and associated air showers simultaneously at Mt. Chacaltaya. Monte Carlo simulations were calculated for the present experimental setup. From comparisons with both results, mechanism of gamma family production, change of interaction model, study of the chemical composition are discussed.
引用
收藏
页码：191 / 193
页数：3
相关论文
共 50 条
  • [21] ANTINEUTRINO BURSTS AND COSMIC-RAY AIR SHOWER EXPERIMENTS
    WEEKES, TC
    PORTER, NA
    ASTRONOMY & ASTROPHYSICS, 1974, 37 (02) : 447 - 449
  • [22] Measuring the UHE cosmic-ray composition with tracking detectors in air-shower arrays
    Bernlohr, K
    ASTROPARTICLE PHYSICS, 1996, 5 (02) : 139 - 146
  • [23] Measuring the UHE cosmic-ray composition with tracking detectors in air-shower arrays
    Max-Planck-Institut fur Kernphysik, Postfach 103980, D-69029 Heidelberg, Germany
    Astropart. Phys., 2 (139-146):
  • [24] AN AIR SHOWER ARRAY DESIGNED FOR COSMIC-RAY VARIATION MEASUREMENTS AND HIGH-ENERGY GAMMA-RAY ASTRONOMY
    MORELLO, C
    NAVARRA, G
    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH, 1981, 187 (2-3): : 533 - 538
  • [25] A measurement of the primary cosmic-ray energy spectrum using the hadronic air shower component
    Hörandel, JR
    Antoni, T
    Apel, WD
    Badea, F
    Bekk, K
    Bercuci, A
    Blümer, H
    Bollmann, E
    Bozdog, H
    Brancus, IM
    Büttner, C
    Chilingarian, A
    Daumiller, K
    Doll, P
    Engler, J
    Fessler, F
    Gils, HJ
    Glasstetter, R
    Haeusler, R
    Haungs, A
    Heck, D
    Holst, T
    Iwan, A
    Kampert, KH
    Kempa, J
    Klages, HO
    Knapp, J
    Maier, G
    Mathes, HJ
    Mayer, HJ
    Milke, J
    Müller, M
    Obenland, R
    Oehlschläger, J
    Petcu, M
    Rebel, H
    Risse, M
    Roth, M
    Schatz, G
    Schieler, H
    Scholz, J
    Thouw, T
    Ulrich, H
    Vulpescu, B
    Weber, JH
    Wentz, J
    Wochele, J
    Zabierowski, J
    PROCEEDINGS OF THE 27TH INTERNATIONAL COSMIC RAY CONFERENCE, 2002, 6693 : 13 - 16
  • [26] Methods of determination of the energy and mass of primary cosmic ray particles at extensive air shower energies
    Kampert, KH
    JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 2001, 27 (07) : 1663 - 1673
  • [27] STRUCTURE AND COMPOSITION OF AIR SHOWER CORES
    KASNITZ, HL
    SITTE, K
    PHYSICAL REVIEW, 1954, 94 (04): : 977 - 987
  • [28] STRUCTURE AND COMPOSITION OF AIR SHOWER CORES
    KASNITZ, HL
    SITTE, K
    PHYSICAL REVIEW, 1953, 90 (02): : 361 - 361
  • [29] Study on the cosmic ray intensity variation using scintillation counters for air shower observation
    Nonaka, Toshiyuki
    Oshima, Akitoshi
    Yamazaki, Katsuya
    37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021, 2022,
  • [30] Simulation of radio emission from cosmic ray air shower with SELFAS2
    Marin, Vincent
    Revenu, Benoit
    ASTROPARTICLE PHYSICS, 2012, 35 (11) : 733 - 741
12345