NONLINEAR EVOLUTION OF MAGNETOPAUSE TEARING MODES

被引:17
作者
CORONITI, FV
QUEST, KB
机构
[1] UNIV CALIF LOS ANGELES,DEPT EARTH & SPACE SCI,LOS ANGELES,CA 90024
[2] UNIV CALIF LOS ANGELES,DEPT MET & CERAM,LOS ANGELES,CA 90024
来源
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1984年 / 89卷 / NA1期
关键词
EARTH ATMOSPHERE - GEOPHYSICS - Magnetic - PLASMAS - Flow;
D O I
10.1029/JA089iA01p00137
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Since the magnetosheath plasma is highly turbulent, reconnection at the dayside magnetopause is likely to be temporally unsteady. The tearing mode can be viewed as a model for the unsteady development of a reconnecting magnetic topology. Magnetopause tearing occurs in the guide-field limit and has a wave packet spatial structure in the east-west direction. This paper presents a solution for the nonlinear evolution of a single wavelength guide-field tearing mode including the effects of finite transit time on the Landau resonant electrons. Short wavelength modes evolve algebraically in time with perturbation amplitudes proportional to t**2. Long wavelength modes are fully nonlinear, and the amplitude grows linearly in time.
引用
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页码:137 / 146
页数:10
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