Observations and models of the fast and slow solar wind

被引：0

作者：

Marsch, E ^{[1
]}

机构：

[1] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany

来源：

31ST ESLAB SYMPOSIUM ON CORRELATED PHENOMENA AT THE SUN, IN THE HELIOSPHERE AND IN GEOSPACE | 1997年 / 415卷

关键词：

sun; corona; EUV emission lines; solar wind; ion and electron temperatures; Alfven waves;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observations and models of the solar wind are reviewed. New important results, from ongoing heliospheric and solar missions, have been obtained by means of in-situ measurements of particles and fields and by remote sensing of the solar atmosphere through imaging and photon spectroscopy. The observations are evaluated in connection with recent modelling efforts to understand theoretically the origin of the solar wind in the three-dimensional corona of the Sun. Special attention will be given to the source region of the steady and fast solar wind originating in the quiet chromosphere and transition region of the polar coronal holes. Acceptable models of the unsteady slow wind, originating in the dynamic equatorial streamer belt from which the global heliospheric current sheet evolves, do presently not exist.

引用

页码：7 / 16

页数：4

共 50 条

[1] Observations and models of the fast and slow solar wind
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[J]. RECENT INSIGHTS INTO THE PHYSICS OF THE SUN AND HELIOSPHERE: HIGHLIGHTS FROM SOHO AND OTHER SPACE MISSIONS, 2001, (203): : 447 - 455
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[J]. ASTRONOMY & ASTROPHYSICS, 2023, 676
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