Heating and Acceleration of the Solar Wind by Ion Acoustic Waves-Parker Solar Probe

被引：2
|
作者：
Kellogg, P. J. [1 ]
Mozer, F. S. [2 ]
Moncuquet, M. [3 ]
Malaspina, D. M. [4 ,5 ]
Halekas, J. [6 ]
Bale, S. D. [2 ]
Goetz, K. [1 ]
机构：
[1] Univ Minnesota, Minnesota Inst Astrophys, Minneapolis, MN USA
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA
[3] LESIA Observ Paris, 5 Pl J Janssen, F-92195 Meudon, France
[4] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO USA
[5] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO USA
[6] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
来源：
ASTROPHYSICAL JOURNAL | 2024年 / 964卷 / 01期
关键词：
PLASMA; TEMPERATURE; TURBULENCE; DENSITY; NOISE;
D O I：
10.3847/1538-4357/ad029f
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The heating of the solar wind has been shown to be correlated with certain ion acoustic waves. Here calculations of the heating are made, using the methods used previously for STEREO observations, which show that the strong damping of ion acoustic waves rapidly delivers their energy to the plasma of the solar wind. It is shown that heating by the observed waves is not only sufficient to produce the observed heating but can also provide much or all of the outward acceleration of the solar wind.
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页数：10
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