Libbrecht, Ken G. (1988) What do the Observations Tell us About the Excitation of Solar Oscillation Modes? In: Advances in Helio- and Asteroseismology. International Astronomical Union Symposium (IAUS). No.123. Springer Netherlands , Dordrecht, pp. 359-362. ISBN 9789027726155. https://resolver.caltech.edu/CaltechAUTHORS:20201008-112317568
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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.
| Item Type: | Book Section | |||||||||
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| Additional Information: | © International Astronomical Union 1988. | |||||||||
| Subject Keywords: | Mode Amplitude; Solar Physics; Oscillation Mode; Convection Zone; Solar Convection Zone | |||||||||
| Series Name: | International Astronomical Union Symposium (IAUS) | |||||||||
| Issue or Number: | 123 | |||||||||
| DOI: | 10.1007/978-94-009-4009-3_73 | |||||||||
| Record Number: | CaltechAUTHORS:20201008-112317568 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20201008-112317568 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 105927 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 08 Oct 2020 19:25 | |||||||||
| Last Modified: | 16 Nov 2021 18:47 |
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