POSSIBLE CONTRIBUTION OF PRIMARY GAMMA-RAYS TO THE OBSERVED COSMIC-RAY ANISOTROPY

被引：16
作者：
ALEXEENKO, VV
NAVARRA, G
机构：
[1] UNIV TURIN,IST FIS GEN,I-10124 TURIN,ITALY
[2] CNR,IST COSMOGEOFIS,TURIN,ITALY
来源：
LETTERE AL NUOVO CIMENTO | 1985年 / 42卷 / 07期
关键词：
D O I：
10.1007/BF02747045
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
引用
收藏
页码：321 / 324
页数：4
相关论文
共 13 条
[1]  
ALEXEENKO VV, 1981, 17TH P INT C COSM RA, V2, P146
[2]  
ALEXENKO VV, 1984, IZV AKAD NAUK SSSR F, V48, P2126
[3]  
BENNETT K, 1977, 12TH P ESLAB S, P83
[4]  
BERGESON HE, 1979, P 16 INT COSM RAY C, V4, P188
[5]  
DAVIES ST, 1979, 16TH P INT COSM RAY, V4, P210
[6]  
FENTON AG, 1976, P INT COSMIC RAY S H, P313
[7]  
GOMBOSI T, 1975, P INT COSMIC RAY C, V4, P1482
[8]  
LAMBERT A, 1983, 18TH INT COSM RAY C, V9, P219
[9]   MODULATION OF GALACTIC COSMIC-RAY ANISOTROPY IN HELIOMAGNETOSPHERE - AVERAGE SIDEREAL DAILY VARIATION [J].
NAGASHIMA, K ;
MORISHITA, I ;
YASUE, S .
PLANETARY AND SPACE SCIENCE, 1982, 30 (09) :879-896
[10]  
Nagashima K., 1976, P INT COSM RAY S HIG, P326
12