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Helioseismology
[摘要] The sun being the nearest star, seismic observations with high spatial resolution are possible, thus providing accurate measurement of frequencies of about half million modes of solar oscillations covering a wide range of degree. With these data helioseismology has enabled us to study the solar interior in sufficient detail to infer the large-scale structure and rotation of the solar interior. With the availability of high quality helioseismic data over a good fraction of a solar cycle it is also possible to study temporal variations in solar structure and dynamics. Some of these problems and recent results will be discussed.
[发布日期]  [发布机构] 
[效力级别]  [学科分类] 天文学(综合)
[关键词] Sun: oscillations;sun: interior;sun: rotation. [时效性] 
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