What we have learned from helioseismology

被引：2
|
作者：
Thompson, MJ [1 ]
机构：
[1] Univ London Queen Mary & Westfield Coll, Sch Math Sci, Astron Unit, London E1 4NS, England
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1998年 / 261卷 / 1-4期
关键词：
D O I：
10.1023/A:1002068719915
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Sun's global oscillations, which are studied both in spatially unresolved ("Sun-as-a-star") and resolved observations of the solar disk, have enabled helioseismology to probe in detail the solar interior. I review first what is learned from the unresolved measurements, since this gives an idea of what we may in the not too distant future be able to learn about the interiors of other stars undergoing solar-type oscillations. I then look at the main results from resolved observations, which have begun to reveal the structure and dynamics of the interior of a star in exquisite detail.
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页码：23 / 34
页数：12
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