Alfven waves in a two-fluid model of the solar wind

Alfven waves in a two-fluid model of the solar wind
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DOI:
10.1086/152072
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发表时间:
1973-04
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
J. V. Hollweg
J. V. Hollweg
中科院分区:
其他
文献类型:
--
作者:
J. V. Hollweg

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本文提出了一个考虑阿尔芬波存在的双流体太阳风模型。这些阿尔芬波的有效压力被认为是,以及通过非线性阿尔芬波阻尼质子加热的模型表示。太阳赤道面自转的影响是允许的。计算结果的影响进行了讨论。
A two-fluid model for the solar wind is presented that includes the presence of Alfven waves which originate at the sun. The effective pressure of these Alfven waves is considered, as well as a model representation for proton heating through nonlinear Alfven wave damping. The effects of rotation in the solar equatorial plane are allowed for. The implications of the computational results obtained are discussed.