The near-earth solar wind

被引：16
|
作者：
Goldstein, ML [1 ]
Eastwood, JP
Treumann, RA
Lucek, EA
Pickett, J
Décréau, P
机构：
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany
[3] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London, England
[4] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[5] CNRS, LPCE, F-75700 Paris, France
[6] Univ Orleans, F-45067 Orleans, France
来源：
SPACE SCIENCE REVIEWS | 2005年 / 118卷 / 1-4期
基金：
美国国家航空航天局;
关键词：
D O I：
10.1007/s11214-005-3823-4
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The solar wind, which is a tenuous ionised gas that carries with it magnetic fields reaching back into the solar atmosphere, is discussed. The wind flows at speeds ranging from a couple of hundred Km s-1 to 1000 Km s-1. The embedded magnetic field has a value of 5 nT. The speed of plasma wave, known as Alfvén waves is also about 40 Km s-1 at 1 AU. The density of this ionised gas at 1 AU is about 5 particles cm -3.
引用
收藏
页码：7 / 39
页数：33
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