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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
Abstract
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.
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- Part 5. Theoretical Models of Classical Pulsating Stars
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- Copyright © Astronomical Society of the Pacific 2000
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