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Why the Chromosphere has Its Discrete Fine Structure

Published online by Cambridge University Press:  14 August 2015

Hermann U. Schmidt
Hermann U. Schmidt*
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, München, Germany

Extract

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The fine structure in the chromosphere is probably controlled by magnetic flux concentrations which cellular convection produces in the photosphere. We will first deal with this flux concentration by the convection and its constraints. Then we will discuss the chromospheric network and its main constituent, the spicules. Following that we will look at the inside of the network, i.e. the fibrils.

Type
Part II: The Quiet Chromosphere: Disk Phenomena
Information
Symposium - International Astronomical Union , Volume 56: Chromospheric Fine Structure , 1974 , pp. 35 - 44
Copyright
Copyright © Reidel 1974 

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