Growth of the Langmuir cavity eigenmodes in the solar wind

S. L. G. Hess; D. M. Malaspina; R. E. Ergun

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Growth of the Langmuir cavity eigenmodes in the solar wind

机译：朗缪尔腔固有模式的增长太阳风

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The Langmuir waves in the solar wind are known to be at the origin of many types of solar radio emissions, in particular solar type II and type III radio bursts. In situ observations have shown that the largest amplitude Langmuir waves often appear as localized wave packets. Several models have been proposed to explain this localization of the waves, such as kinetic localization, nonlinear wave-wave processes, or eigenmode formation. The latter theory states that the wave packets are eigenmodes of density cavities generated by background turbulence. In the present paper we investigate the wave growth of the localized Langmuir eigenmodes.

机译：朗缪尔波在太阳风是已知的在许多类型的太阳射电的起源排放,特别是太阳能II型和类型三世无线电脉冲。经常的最大振幅波朗缪尔表现为局部的波包。提出了解释这个本地化吗波,如动力定位、非线性波波流程或固有模式形成。数据包是密度腔的固有模式湍流产生的背景。本文我们研究波的增长本地化朗缪尔固有模式。

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《Journal of Geophysical Research, A. Space Physics: JGR》 |2010年第10期|A10103:1-A10103:8|共8页
作者
S. L. G. Hess; D. M. Malaspina; R. E. Ergun;
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作者单位

LASP, University of Colorado at Boulder, Boulder, Colorado, USA;

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原文格式 PDF
正文语种英语
中图分类空间物理;
关键词
Langmuir; waves; solar windWave packetsplasma Langmuir waves;

机译：朗缪尔;波浪;太阳风波包等离子体朗缪尔波;

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8. Localized Langmuir Eigenmodes and Solar Radio Bursts [O] . ^D. M. Malaspina 2011

机译：本地化的Langmuir eigenmodes和太阳型无线电爆发
9. MOTHRA:A CAVITY EIGENMODE CODE FOR NONUNIFORM MAGNETIZED PLASMA [R] . CHENG CHU, J. L. SPERLING 1978

机译：mOTHRa：用于非均匀磁化等离子体的CaVITY EIGENmODE代码

Growth of the Langmuir cavity eigenmodes in the solar wind

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