TRANSMISSION AND DAMPING OF HYDROMAGNETIC-WAVES BEHIND A STRONG SHOCK FRONT - IMPLICATIONS FOR COSMIC-RAY ACCELERATION

被引：48

作者：

ACHTERBERG, A

BLANDFORD, RD

机构：

[1] CALTECH,PASADENA,CA 91125

[2] ASTRON INST UTRECHT,3512 NL UTRECHT,NETHERLANDS

来源：

关键词：

D O I：

10.1093/mnras/218.3.551

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：551 / 575

页数：25

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[3]

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[4]

ANDERSON YE, 1963, MAGNETOHYDRODYNAMIC

[5]

Axford W. I., 1981, Plasma Astrophysics Course and Workshop (ESA-SP-161), P425

[6] ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1. [J].

BELL, AR .

[7]

BLANDFORD RD, 1985, UNPUB PHYS REPTS

DRURY, LOC .

[9]

KENNEL CF, 1984, P CHAPMAN C COLLISIO

[10]

Krall N. A., 1983, PRINCIPLES PLASMA PH