PARTICLE-ACCELERATION IN A MHD SIMULATION OF MAGNETOTAIL DYNAMICS

被引:0
|
作者
BIRN, J [1 ]
HESSE, M [1 ]
机构
[1] NASA, GODDARD SPACE FLIGHT CTR, ELECTRODYNAM BRANCH, GREENBELT, MD 20771 USA
来源
ADVANCES IN SPACE RESEARCH-SERIES | 1993年 / 13卷 / 04期
关键词
D O I
暂无
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The acceleration of protons in a dynamically evolving magnetotail is investigated on the basis of a three-dimensional resistive MHD simulation and the tracing of particles in the fields obtained from that simulation. The MHD simulation, representing plasmoid formation and ejection through a near-Earth reconnection process, generates cross-tail electric fields of up to about 4-mV/m, which lead to integrated potential differences across the tail of up to 200-kV. The large spatial extent of the increased electric field, which is largely associated with the plasma motion, together with the finite cross-tail extent suggest that acceleration might take place over a wide range of locations in x. This is confirmed by the particle tracing. An investigation of energized particles in the near-Earth region shows that these particles occupy a significant portion of the closed field line region inside of, but for moderate energies of tens of keV, not directly adjacent to, the separatrix.
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页码:245 / 248
页数:4
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