On the excitation of solar 5-minute oscillations

Antia, H. M. ; Chitre, S. M. ; Gough, D. O. (1987) On the excitation of solar 5-minute oscillations Proceedings of the International Astronomical Union Symposium No. 123 on Advances in Helio- and Astero-seismology . pp. 371-374.

PDF - Publisher Version

Official URL: http://articles.adsabs.harvard.edu/cgi-bin/nph-iar...


A simple prescription for the dynamics of convection perturbed by stellar pulsation is used in an estimation of the growth rates of solar five-minute modes. Convection appears to enhance the excitation of the modes, and the maximum in the growth rate versus frequency found previously when oscillatory convective perturbations were ignored is still present.

Item Type:Article
Source:Copyright of this article belongs to International Astronomical Union.
ID Code:75631
Deposited On:24 Dec 2011 13:59
Last Modified:18 May 2016 19:35

Repository Staff Only: item control page