ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1.

被引:2324
作者
BELL, AR [1 ]
机构
[1] MULLARD RADIO ASTRON OBSERV,CAVENDISH LAB,CAMBRIDGE CB3 0HE,ENGLAND
关键词
D O I
10.1093/mnras/182.2.147
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:147 / 156
页数:10
相关论文
共 13 条
[1]  
Boyd T. J., 1969, PLASMA DYNAMICS
[2]   NONLINEAR DISSIPATION OF ALFVEN WAVES [J].
CHIN, YC ;
WENTZEL, DG .
ASTROPHYSICS AND SPACE SCIENCE, 1972, 16 (03) :465-&
[3]   INCREASES IN LOW-ENERGY COSMIC RAY INTENSITY AT FRONT OF PROPAGATING INTERPLANETARY SHOCK WAVES [J].
FISK, LA .
JOURNAL OF GEOPHYSICAL RESEARCH, 1971, 76 (07) :1662-+
[4]  
FORMISANO V, 1974, CORRELATED INTERPLAN
[5]  
GREENSTADT EW, 1975, MAGNETOSPHERES EARTH
[6]  
Hudson P D., 1965, MON NOT ROY ASTRON S, V131, P23, DOI DOI 10.1093/MNRAS/131.1.23
[8]  
KULSRUD RM, 1971, ASTROPHYS LETT COMM, V8, P189
[9]   RATIO OF SPECIFIC HEATS IN SOLAR-WIND PLASMA FLOW THROUGH EARTHS BOW SHOCK [J].
SHEN, WW .
JOURNAL OF GEOPHYSICAL RESEARCH, 1971, 76 (34) :8181-+
[10]   COSMIC-RAY STREAMING .3. SELF-CONSISTENT SOLUTIONS [J].
SKILLING, J .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1975, 173 (02) :255-269