ION CYCLOTRON RESONANT INSTABILITY OF RH WAVES PROPAGATING AT AN ANGLE TO INTERPLANETARY MAGNETIC FIELD

被引：7

作者：

CUPERMAN, S

LANDAU, RW

机构：

[1] Dept. of Physics and Astronomy, Tel-Aviv University, Tel-Aviv

[2] The Institute of Planetary and Space Science, Tel-Aviv University, Tel-Aviv

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1969年 / 5卷 / 03期

关键词：

D O I：

10.1007/BF00650000

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The anomalous Doppler-shift interaction between positive ions and right-hand (RH) polarized E.M. waves propagating at a small angle to a static magnetic field is investigated. The linear rate of growth of the resulting instability is obtained and compared with the growth rate for the parallel propagation case. For conditions typical of the solar wind at about 1 AU, the rate of growth always decreases with increasing propagation angle. For very large ion pressures (β{norm of matrix}≫1) and temperature anisotropies (T{norm of matrix}T⊥≫1), the rate of growth may increase with increasing propagation angle. © 1969 D. Reidel Publishing Company.

引用

页码：333 / &