Fast evolving spatial structure of auroral parallel electric fields

被引:31
作者
Génot, V
Louarn, P
Mottez, F
机构
[1] Queen Mary Univ London, Astron Unit, London E1 4NS, England
[2] Ctr Etud Spatiale Rayonnements, F-31400 Toulouse, France
[3] Cte Etud Environm Terr & Planetaires, F-78140 Velizy Villacoublay, France
关键词
D O I
10.1029/2001JA000076
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use a new nonlinear guiding center particle in cell code to investigate the role of Alfven waves in the auroral particle acceleration. The propagation of an Alfven wave in an inhomogeneous auroral plasma, described by a density cavity, is considered. Parallel electric fields are generated on the edges of the cavity, leading to an efficient electron acceleration and to the formation of electron beams. A beam-plasma instability takes place. It evolves nonlinearly, and small-scale electrostatic structures are created and propagate at a velocity close to the Alfven velocity. A first category of these structures could be assimilated to weak double layers, whereas a second may be related to electron phase space holes. This study demonstrates the potential importance of Alfven waves in the auroral acceleration and the coupling between large-scale electromagnetic and small-scale electrostatic phenomena.
引用
收藏
页码:29633 / 29643
页数:11
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