ELECTROMAGNETIC ION-CYCLOTRON WAVES IN THE PLASMA DEPLETION LAYER

被引:47
作者
DENTON, RE
HUDSON, MK
FUSELIER, SA
ANDERSON, BJ
机构
[1] DARTMOUTH COLL, DEPT PHYS & ASTRON, HANOVER, NH 03755 USA
[2] LOCKHEED PALO ALTO RES LABS, PALO ALTO, CA 94304 USA
[3] JOHNS HOPKINS UNIV, APPL PHYS LAB, LAUREL, MD 20707 USA
关键词
D O I
10.1029/93JA00796
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have studied the theoretical properties of electromagnetic ion cyclotron (EMIC) waves which occur in the plasma depletion layer. Our analysis assumes a homogene-s plasma with the characteristics which were measured by the AMPTE/CCE satellite at 1450-1 501 UT on October 5, 1984. During this time, waves were observed in the Pc 1 frequency range (0.2-5 Hz) below the hydrogen gyrofrequency, and we identify these waves as EMIC waves. In agreement with observations, the theory predicts two frequency bands of waves, above and below about 0.4 OMEGA(H), where OMEGA(H) is the hydrogen gyrofrequency. The higher-frequency instability is driven by the temperature anisotropy of the H+ ions, while the lower-frequency instability is driven by the temperature anisotropy of the He-2+ ions. These two frequency bands occur on the same dispersion surface. The EMIC waves tend to quasi-linearly control the value of the proton temperature ratio T(perpendicular-to)/T(parallel-to) by an increase in T(parallel-to) due to scattering so that the bulk plasma stays near marginal stability. Here, T(parallel-to) (T(perpendicular-to)) is the temperature parallel (perpendicular) to B0. Without convective effects, the nonlinear wave amplitude tends to be large over the entire angular range 0 < theta(kB) less-than-or-equal-to 75-degrees, where theta(kB) is the angle between the wave vector and the background magnetic field (B0). However, waves for which the perpendicular (to B0) group velocity v(g perpendicular-to) is large, are likely to be convectively limited in growth. Within the higher-frequency band, v(g perpendicular-to) is small only for wave vectors k which are close to parallel to B0. Within the lower-frequency band, v(g perpendicular-to) is small only for oblique k. Therefore, it is likely that the higher-frequency waves will have k roughly parallel to B0 and will be left-hand polarized, while the lower-frequency wave band will have k oblique to B0 and will be linearly polarized, in agreement with observations.
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页码:13477 / 13490
页数:14
相关论文
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