F' SPECTRUM OF HIGH-ENERGY GAMMA-RAY FAMILIES

被引：3

作者：

AKASHI, M

NANJO, H

WATANABE, Z

OHTA, I

MISAKI, A

MIZUTANI, K

KASAHARA, K

KONISHI, E

TORII, S

YUDA, T

MITO, I

SHIRAI, T

TATEYAMA, N

TAIRA, T

SHIBATA, M

SUGIMOTO, H

TAIRA, K

机构：

[1] SAITAMA UNIV,DEPT PHYS,SAITAMA,JAPAN

[2] SHIBAURA INST TECHNOL,SHIBAURA,TOKYO,JAPAN

[3] SAGAMI INST TECHNOL,KANAGAWA,JAPAN

[4] UTSUNOMIYA UNIV,FAC EDUC,TOCHIGI,JAPAN

[5] UNIV TOKYO,COSM RAY LAB,TANASHI,TOKYO,JAPAN

[6] KANAGAWA UNIV,FAC ENGN,YOKOHAMA,JAPAN

[7] UNIV LODZ,INST PHYS,PL-90237 LODZ,POLAND

来源：

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 1978年 / 4卷 / 02期

关键词：

D O I：

10.1088/0305-4616/4/2/006

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

引用

页码：L41 / L44

页数：4

共 12 条

[1]

AKASHI M, 1975, 14TH P INT C COSM RA, V7, P2555

[2]

AKASHI M, 1977, 15TH P INT C COSM RA, V7, P190

[3]

Baradzey L.T., 1970, T FIAN, V46, P200

[4]

DUNAEVSKY AM, 1977, 15TH P INT C COSM RA, V7, P354

[5]

FOMIN YA, 1977, 15 P INT COSM RAY C, V7, P248

[6] CAN WE UNDERSTAND HIGH-ENERGY COSMIC-RAY SPECTRA ON BASIS OF SCALING HYPOTHESIS [J].

KASAHARA, K ;

TAKAHASHI, Y .

PROGRESS OF THEORETICAL PHYSICS, 1976, 55 (06) :1896-1911

[7]

KASAHARA K, 1977, 15TH P INT C COSM RA, V7, P236

[8]

KASAHARA K, 1973, 13TH P INT C COSM RA, V3, P2305

[9]

KEMPA J, 1977, 15TH INT C COSM RAYS

[10]

TOMASZEWSKI A, 1977, 15TH P INT C COSM RA, V7, P255

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