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Waves and Oscillations in the Non-Magnetic Photosphere

Published online by Cambridge University Press:  08 February 2017

Franz - Ludwig Deubner
Franz - Ludwig Deubner*
Affiliation:
Institut für Astronomie und Astrophysik der Universität Würzburg Am Hubland, D-8700 Würzburg

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The solar photosphere is the outer boundary of the cavity which defines the spectrum of the global p-modes. It is also the lowest layer that permits direct observation of the boiling mixture of motions which eventually create the complex patterns apparent in the chromosphere and corona. Studies of the dynamical behaviour of this layer are therefore of paramount importance for an overall understanding of the dynamic sun.

Type
IV. Magnetohydrodynamics of the Photosphere
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 217 - 228
Copyright
Copyright © Kluwer 1990 

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