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Detection of Solar Five-Minute Oscillations of Low Degree*

Published online by Cambridge University Press:  12 April 2016

Philip H. Scherrer ,
John M. Wilcox ,
J. Christensen-Dalsgaard  and
D.O. Gough
Philip H. Scherrer
Affiliation:
Institute for Plasma Research, Stanford University, Stanford, CA 94305, U.S.A.
John M. Wilcox
Affiliation:
Institute for Plasma Research, Stanford University, Stanford, CA 94305, U.S.A.
J. Christensen-Dalsgaard
Affiliation:
National Center for Atmospheric Research, Boulder, CO 80307, U.S.A.
D.O. Gough
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, U.K.

Abstract

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Solar five-minute oscillations of degree l = 3, 4, and 5 have been observed at Stanford, in the Doppler shift of the Fe 5124 line. The frequencies and amplitudes are in broad agreement with previous observations of modes with l ≤ 3, though we note that there are some systematic discrepancies between the results of different observers.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 66: Problems of Solar and Stellar Oscillations , 1983 , pp. 75 - 87
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.

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