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Oscillatory modes of energy transport in solar magnetic regions∗

Published online by Cambridge University Press:  14 August 2015

R. E. Danielson  and
B. D. Savage
R. E. Danielson
Affiliation:
Princeton University Observatory, Princeton, N.J., U.S.A.
B. D. Savage
Affiliation:
Princeton University Observatory, Princeton, N.J., U.S.A.

Abstract

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It appears that it is necessary to look for oscillatory (i.e. overstable) instabilities as the cause of energy transport in sunspots. Making use of recent calculations on the hydromagnetic stability of thermally unstable layers with open boundary conditions, it is found that oscillatory modes can occur in the interior of sunspots. Some possible consequences of these oscillatory modes are discussed.

Type
Part II: Theoretical Aspects
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 112 - 125
Copyright
Copyright © Reidel 1968 

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