Antia, H. M. (2009) The solar interior Current Science, 97 (6). pp. 911-923. ISSN 0011-3891
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Abstract
The sun being the nearest star, provides us a unique opportunity to study stellar processes in sufficient detail to test theories of stellar structure and evolution. Although the solar interior is not directly accessible to observations, development of helioseismology during the last three decades has enabled us to study the structure and dynamics of solar interior with unprecedented accuracy. Some of these developments are described in this article.
| Item Type: | Article |
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| Source: | Copyright of this article belongs to Current Science Association. |
| Keywords: | Helioseismology; Nutrino Fluxes; Solar Interior; Standard Solar Model |
| ID Code: | 75625 |
| Deposited On: | 24 Dec 2011 15:12 |
| Last Modified: | 18 May 2016 19:34 |
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