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Spectral-Spatial Analysis of Wave Motions in the Region of Temperature Minimum of the Sun’s Atmosphere*

Published online by Cambridge University Press:  12 April 2016

V.E. Merkulenko ,
V.I. Polyakov ,
L.E. Palamarchuk  and
N.V. Larionov
V.E. Merkulenko
Affiliation:
SibIZMIR, Siberian Department, USSR Academy of Sciences, Irkutsk 33, P.O. Box 4, U.S.S.R.
V.I. Polyakov
Affiliation:
SibIZMIR, Siberian Department, USSR Academy of Sciences, Irkutsk 33, P.O. Box 4, U.S.S.R.
L.E. Palamarchuk
Affiliation:
SibIZMIR, Siberian Department, USSR Academy of Sciences, Irkutsk 33, P.O. Box 4, U.S.S.R.
N.V. Larionov
Affiliation:
SibIZMIR, Siberian Department, USSR Academy of Sciences, Irkutsk 33, P.O. Box 4, U.S.S.R.

Abstract

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A spectral-spatial analysis is made in the region of temperature minimum of the Sun's atmosphere. Filtergrams in the Ba II 4554 + 0.05 Å line have been used. The wavelengths corresponding to the sequence of peaks on the spectrum are in close agreement with those theoretically calculated by Ulrich and Rhodes (1977) for five-minute oscillations. We thus have good cause to surmize that the observed oscillations in the region of temperature minimum pertain to the p-mode class of general oscillations of the Sun, the main fraction of their energy falling on the period of 300 s.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 66: Problems of Solar and Stellar Oscillations , 1983 , pp. 157 - 161
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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