Heating of the Solar Wind by Ion Acoustic Waves

被引：10

作者：

Kellogg, Paul J. ^{[1
]}

机构：

[1] Univ Minnesota, Minneapolis, MN 55455 USA

来源：

ASTROPHYSICAL JOURNAL | 2020年 / 891卷 / 01期

基金：

美国国家航空航天局;

关键词：

Heliosphere; Solar wind; Solar coronal heating; ASTROPHYSICAL GYROKINETICS; INTERSTELLAR TURBULENCE; PARAMETRIC-EXCITATION; DENSITY-FLUCTUATIONS; FINITE-AMPLITUDE; ALFVEN-WAVE; PLASMA; DISSIPATION; INSTABILITY;

D O I：

10.3847/1538-4357/ab7003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Calculations are made of the energy supplied to the solar wind by the rapid decay of density fluctuations, identified as ion acoustic waves. It is shown that this process supplies an appreciable fraction, perhaps nearly all, of the observed heating of the solar wind. This process may be an important step in the conversion of magnetic turbulence to particle energy.

引用

页数：7

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