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Short Period Oscillations*

Published online by Cambridge University Press:  12 April 2016

F.-L. Deubner  and
J. Laufer
F.-L. Deubner
Affiliation:
Institut für Astronomie und Astrophysik, D-8700 Würzburg, F.R.G.
J. Laufer
Affiliation:
Institut für Astronomie und Astrophysik, D-8700 Würzburg, F.R.G.

Abstract

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Short period oscillations (with periods less than 150 s) are shown to be non-uniformly distributed on the solar surface, and in time. Rather, they appear concentrated in short bursts which preferentially occur in regions with strong instantaneous downflow motion throughout the observed extent of the solar atmosphere.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 66: Problems of Solar and Stellar Oscillations , 1983 , pp. 151 - 155
Copyright
Copyright © Reidel 1983

Footnotes

*

Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.

References

Deubner, F.-L.: 1974, Solar Phys. 39, 31.CrossRefGoogle Scholar
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Deubner, F.-L. and Durrant, C.J.: 1982, Astron. Astrophys., in press.Google Scholar
Evans, J.W. and Michard, R.: 1962, Astrophys. J. 136, 493.CrossRefGoogle Scholar
Howard, R. and Livingston, W.G: 1968, Solar Phys. 3, 434.CrossRefGoogle Scholar