COSMIC-RAY INTENSITY GRADIENTS IN SOLAR-SYSTEM

被引：28

作者：

MCKIBBEN, RB ^{[1
]}

机构：

[1] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637

来源：

关键词：

D O I：

10.1029/RG013i003p01088

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

引用

页码：1088 / &

共 59 条

[1] ANTONUCCI E, 1974, GEOPHYS RES LETT, V1, P302
[2] AXFORD WI, TO BE PUBLISHED
[3] EVIDENCE FOR A COSMIC RAY GRADIENT PERPENDICULAR TO SOLAR EQUATORIAL PLANE
BARKER, MC
HATTON, CJ
[J]. PLANETARY AND SPACE SCIENCE, 1971, 19 (06) : 549 - &
[4] BERCOVITCH M, 1971, 12 P INT C COSM RAYS, V2, P579
[5] SOLAR-WIND VELOCITY FROM IPS OBSERVATIONS
COLES, WA
MAAGOE, S
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (28): : 5622 - +
[6] DORMAN LI, 1973, 13TH INT C COSM RAYS, V2, P713
[7] DORMAN LI, 1973, 13TH P INT COSM RAY, V2, P721
[8] RADIAL GRADIENT OF GALACTIC PROTONS IN INNER SOLAR SYSTEM
ENGLADE, RC
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1971, 76 (34): : 8394 - &
[9] Fan C. Y., 1970, Acta Physica Academiae Scientiarum Hungaricae, V29, P261
[10] MEASUREMENTS OF JOVIAN RADIATION BELTS
FILLIUS, RW
MCILWAIN, CE
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1974, 79 (25): : 3589 - 3599