Antia, H. M. ; Basu, Sarbani (1996) Effect of turbulent pressure on solar oscillation frequencies Proceedings of Solar Convection and Oscillations and their Relationship . pp. 51-54.
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Abstract
We use observed frequencies of solar p-modes to test different formulations for calculating the convective flux. In particular, models using the usual mixing length theory and the formulation of Canuto and Mazzitelli for calculating the convective flux are compared to find that the latter yields frequencies that are closer to observed values. Inclusion of turbulent pressure is also found to improve the agreement with observed frequencies, but the magnitude of the difference is much smaller.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Proceedings of Solar Convection and Oscillations and their Relationship. |
| ID Code: | 75643 |
| Deposited On: | 24 Dec 2011 15:02 |
| Last Modified: | 24 Dec 2011 15:02 |
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