Resonant Excitation of the Solar g-modes Through Coupling of 5-min Oscillations
It is proposed that the interacting solar g-modes are driven by the beat forcing of g-modes by two 5-min oscillations, excited by a к-mechanism. The observational implications of the proposed mechanism are discussed.
KeywordsSolar Phys Beat Frequency Resonant Excitation Turbulent Convection Radial Order
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