Auroral particle acceleration by waves

被引:8
作者
Bingham, R [1 ]
Cairns, RA
Dendy, RO
Shapiro, VD
Shukla, PK
Stenflo, L
机构
[1] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
[2] Univ St Andrews, St Andrews KY16 9SS, Fife, Scotland
[3] AEA Technol Fus, Culham Lab, Abingdon OX14 3DB, Oxon, England
[4] Univ Calif San Diego, Dept Phys, San Diego, CA 92103 USA
[5] Ruhr Univ Bochum, Inst Theoret Phys 4, D-44780 Bochum, Germany
[6] Umea Univ, Dept Plasma Phys, S-90187 Umea, Sweden
来源
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE | 2001年 / 26卷 / 1-3期
基金
美国国家航空航天局;
关键词
D O I
10.1016/S1464-1917(00)00099-4
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The role of waves in accelerating both electrons and ions in the auroral zone is discussed. Various wave generation mechanisms and acceleration processes including acceleration within cavitons and nonlinear potential structures are analysed. The wave modes which we consider include waves such as kinetic Alfven waves, and lower-hybrid waves. In some cases wave amplitudes are found to be large enough for strong turbulence effect to play a significant role in the particle dynamics. These effects manifest themselves in the formation of caviton structures and large scale density striations creating local acceleration regions. A theoretical description of the different nonlinear processes responsible for plasma modification and acceleration will be presented. (C) 2001 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:133 / 144
页数:12
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