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Excitation and Damping of P-Modes
Published online by Cambridge University Press: 08 February 2017
Extract
Millions of seismic eigenmodes are excited to low amplitudes in the Sun, with an amplitude spectrum that grows approximately as a power of the frequency until it reaches a maximum at 3 mHz, and then drops off again towards higher frequencies (Libbrecht, 1988; Libbrecht & Woodard, 1991).
- Type
- IV. Solar Small-Scale Structure
- Information
- Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 199 - 212
- Copyright
- Copyright © Kluwer 1998