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The new solar corona

被引：94
作者：
Aschwanden, MJ [1 ]
Poland, AI
Rabin, DM
机构：
[1] Lockheed Martin Adv Technol Ctr, Solar & Astrophys Lab, Palo Alto, CA 94304 USA
[2] NASA, Goddard Space Flight Ctr, Astron & Solar Phys Lab, Greenbelt, MD 20771 USA
来源：
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 2001年 / 39卷
关键词：
magnetic fields; plasma dynamics; coronal heating; solar flares; coronal mass ejections; extreme ultraviolet; soft X rays;
D O I：
10.1146/annurev.astro.39.1.175
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We focus on new observational capabilities (Yohkoh, SoHO, TRACE), observations, modeling approaches, and insights into physical processes of the solar corona. The most impressive new results and problems discussed in this article can be appreciated from the movies available on the Annual Reviews website and at http://www.Imsal.com/pub/araa/araa.html.
引用
收藏
页码：175 / 210
页数：44
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