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The Effect of the Solar Cycle on the Resonant Coupling of g Modes

Published online by Cambridge University Press:  12 April 2016

C. Jordinson  and
D. O. Gough
C. Jordinson
Affiliation:
Institute of Astronomy, University of Cambridge, UK
D. O. Gough
Affiliation:
Institute of Astronomy and DAMTP, University of Cambridge, UK

Abstract

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We consider the effect of the solar cycle on g-mode parametric resonance, and hence on the limiting amplitude of the overstable solar g1(ℓ = 1) mode. We find no change in the expected limiting amplitude from that found by Dziembowski (1983), who ignored cycle variations.

Type
Part 5. Theoretical Models of Classical Pulsating Stars
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 390
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Dilke, F.W.W. & Gough, D.O. 1972, Nature, 240, 262 CrossRefGoogle Scholar
Dziembowski, W. 1983, Solar Phys., 82, 259 CrossRefGoogle Scholar