Wave-particle interaction in the terrestrial ion foreshock:: new results from Cluster

被引:0
|
作者
Mazelle, C. [1 ]
Meziane, K. [2 ]
Wilber, M. [3 ]
Le Quedau, D. [4 ]
机构
[1] UPS CNRS, Ctr Etud Spatiale Rayonnements, 9 Ave Colonel Roche, F-31400 Toulouse, France
[2] Univ New Brunswick, Dept Phys, Fredericton, NB, Canada
[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[4] Inst Natl Sci Univ, F-75794 Paris, France
来源
TURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS | 2007年 / 932卷
关键词
planetary bow shock; ion foreshock; wave-particle interaction;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Different types of backstreaming ion distributions have been reported in the region upstream from the Earth's bow shock and magnetically connected to it (ion foreshock): field-aligned beams (FABs), gyrating ion and diffuse ion distributions. Contrary to the first type, the two others are always associated with ULF waves. Among them, gyrating ions with well-defined pitch-angle and gyrophase organization around the local magnetic field have been frequently observed in association with large amplitude quasi-monochromatic right-hand mode waves. These waves reveal the existence of coherent wave-particle interaction which is an efficient process to dissipate the energy of the particles reflected at the collisionless bow shock. It has been shown recently from a large data set from multi-spacecraft observations by Cluster that the gyrophase-bunched ion distributions are mainly produced by such a process from cyclotron-resonant FABs observed just both at the edge of the gyrating ions region and the boundary of ULF waves.
引用
收藏
页码:175 / +
页数:2
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