Antia, H. M. (2003) Does the sun shrink with increasing magnetic activity? Astrophysical Journal, 590 (1). pp. 567-572. ISSN 0004-637X
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Official URL: http://iopscience.iop.org/0004-637X/590/1/567?from...
Related URL: http://dx.doi.org/10.1086/374916
Abstract
It has been demonstrated that frequencies of f-modes can be used to estimate the solar radius to a good accuracy. These frequencies have been used to study temporal variations in the solar radius with conflicting results. The variation in f-mode frequencies is more complicated than what is assumed in these studies. If a careful analysis is performed, then it turns out that there is no evidence for any variation in the solar radius.
Item Type: | Article |
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Source: | Copyright of this article belongs to American Astronomical Society. |
ID Code: | 12391 |
Deposited On: | 10 Nov 2010 06:17 |
Last Modified: | 16 May 2016 21:44 |
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