Published 1988
| public
Book Section - Chapter
What do the Observations Tell us About the Excitation of Solar Oscillation Modes?
- Creators
- Libbrecht, Ken G.
Chicago
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Abstract
Present theories suggest two different classes of excitation mechanisms which may be responsible for the observed amplitudes of solar p-mode oscillations—self-excitation of the modes (e.g. the κ mechanism), and stochastic excitation by turbulent convection. I discuss here the agreement and disagreement between the predictions of these two mechanisms and the observed mode amplitudes and linewidths.
Additional Information
© International Astronomical Union 1988.Additional details
- Eprint ID
- 105927
- Resolver ID
- CaltechAUTHORS:20201008-112317568
- Created
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2020-10-08Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Series Name
- International Astronomical Union Symposium (IAUS)
- Series Volume or Issue Number
- 123