Periods and stability of solar g-modes

Details Periods and stability of solar g-modes Periods and stability of solar g-modes

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128..123c&link_type=abstract

(IAU, The Inside the Sun Colloquium, 121st, Versailles, France, May 22-26, 1989) Solar Physics (ISSN 0038-0938), vol. 128, July

Physics

4

Convection Currents, Solar Gravitation, Solar Oscillations, Stellar Models, Periodic Variations, Solar Neutrinos, Weak Interactions (Field Theory)

Scientific paper

The g-mode frequencies are presented for two models, the Cox, Guzik, and Kidman (CGK) model and the Cosmion 1 case of the Cox, Guzik, and Raby (CGR) model. It is found that the observed g-mode frequencies fit current standard models and are particularly close to the CGK model, Neither mixed-in hydrogen models nor models relying on considerable conduction from Cosmions match the p- and g-mode data as well.

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