Antia, H. M. ; Chitre, S. M. (1991) Theoretical spectrum of solar convection Proceedings of the Conference on "Challenges to Theories of the Structure of Moderate Mass Stars", Santa Barbara . pp. 157-162.
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Abstract
The theoretical power spectrum of solar velocity field and flux variation is obtained with amplitudes of the unstable convective eigenmodes determined by linearly superposing these modes to yield the model convective flux profile. The numerical results are compared with the observed spectrum of solar convection and the technique is applied to other stars.
Item Type: | Article |
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Source: | Copyright of this article belongs to Proceedings of the Conference on "Challenges to Theories of the Structure of Moderate Mass Stars", Santa Barbara. |
ID Code: | 75636 |
Deposited On: | 24 Dec 2011 14:01 |
Last Modified: | 12 Jul 2012 08:41 |
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