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Excitation and Damping of P-Modes

Published online by Cambridge University Press:  08 February 2017

Åke Nordlund  and
Robert F. Stein
Åke Nordlund
Affiliation:
Theoretical Astrophysics Center, and Astronomical Observatory / NBIfAFG, Juliane Maries Vej 30, 2100 Copenhagen Ø, Denmark
Robert F. Stein
Affiliation:
Dept. of Physics and Astronomy, Michigan State University, East Lansing, MI 48823, U.S.A.

Extract

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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 

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