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Waves and Oscillations in the Non-Magnetic Photosphere
Published online by Cambridge University Press: 08 February 2017
Extract
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
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- Copyright © Kluwer 1990
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