Solar Wind Electron Energization by Plasma Turbulence

被引：7
|
作者：
Yoon, P. H. [1 ,2 ]
机构：
[1] Univ Maryland, IPST, College Pk, MD 20742 USA
[2] Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi, South Korea
来源：
14TH ANNUAL INTERNATIONAL ASTROPHYSICS CONFERENCE: LINEAR AND NONLINEAR PARTICLE ENERGIZATION THROUGHOUT THE HELIOSPHERE AND BEYOND | 2015年 / 642卷
基金：
美国国家科学基金会;
关键词：
VELOCITY DISTRIBUTION-FUNCTIONS; GLOBAL PROCESSES; THERMAL NOISE; CORONA; WAVES; SUPPORT; ORIGIN; MODEL;
D O I：
10.1088/1742-6596/642/1/012030
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The solar wind electrons are made of the low-energy Maxwellian core, intermediateenergy halo, field-aligned strahl, and the highly-energetic super-halo electrons. The present paper discusses a model in which the halo electrons interact with the whistler fluctuation via cyclotron wave-particle resonance, and the super-halo electrons interact through Landau resonance with the Langmuir fluctuation, thus maintaining a local steady state.
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页数：6
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