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

页码：321 / 324

页数：4

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
NAGASHIMA, K
MORISHITA, I
YASUE, S
[J]. PLANETARY AND SPACE SCIENCE, 1982, 30 (09) : 879 - 896
[10] Nagashima K., 1976, P INT COSM RAY S HIG, P326