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On the Existence of Hydromagnetic Interface Waves at a Structured Atmosphere
Published online by Cambridge University Press: 19 July 2016
Abstract
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The conditions under which the hydromagnetic interface waves can exist at a magnetic interface is deduced. Using these conditons, it is shown that a slow interface wave with a phase velocity about 5Km/s and a fast interface wave with a phase velocity 6.5 to 8km/s at the photospheric level can exist.
- Type
- VI. Chromospheric and Coronal Heating
- Information
- Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 262 - 263
- Copyright
- Copyright © Kluwer 1990