期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 328, 期 1-2, 页码 43-50出版社
SPRINGER
DOI: 10.1007/s10509-009-0201-9
关键词
Sun: helioseismology; Sun: abundances; Sun: activity
资金
- NSF [ATM 0348837, ATM 073770]
- Div Atmospheric & Geospace Sciences
- Directorate For Geosciences [0737770] Funding Source: National Science Foundation
Helioseismology has given us a unique window into the solar interior. Helioseismic data have enabled us to study the internal structure and dynamics with unprecedented detail. This has also allowed us to use the Sun as a laboratory to study the basic properties of stellar matter. We describe how helioseismology is used to determine solar structure and what we have learned about the Sun so far. We also describe how knowledge of the solar structure can be used to constrain the physics inputs.
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