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Oscillatory modes of energy transport in solar magnetic regions∗
Published online by Cambridge University Press: 14 August 2015
Abstract
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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