UVCS/SOHO: The first two years

被引：9

作者：

Cranmer, SR

Kohl, JL

Noci, G

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[2] Univ Florence, I-50125 Florence, Italy

来源：

SPACE SCIENCE REVIEWS | 1998年 / 85卷 / 1-2期

关键词：

corona; solar wind; UV radiation; spectroscopy; line profiles;

D O I：

10.1023/A:1005175106042

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) has observed the extended solar corona between 1 and 10 R. for more than two years. We review spectroscopic and polarimetric measurements made in coronal holes, equatorial streamers, and coronal mass ejections, as well as selected non-solar targets. UVCS/SOHO has provided a great amount of empirical information about the physical processes that heat and accelerate the solar wind, and about detailed coronal structure and evolution.

引用

页码：341 / 348

页数：8

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