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Solar and Stellar Magnetic Fields and Atmospheric Structures: Theory*

Published online by Cambridge University Press:  12 April 2016

E. N. Parker
E. N. Parker*
Affiliation:
Enrico Fermi Institute, Depts. Physics and Astronomy, University of Chicago, Chicago, IL 60637, U.S.A.

Abstract

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This presentation reviews selected ideas on the origin of the magnetic field of the Sun, the dynamical behavior of the azimuthal field in the convective zone, the fibril state of the field at the photosphere, the formation of sunspots, prominences, the spontaneous formation of current sheets in the bipolar field above the surface of the Sun, coronal heating, and flares.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 104 , Issue 1: Solar and Stellar Flares , 1989, pp. 271 - 288
Copyright
Copyright © Kluwer 1989

Footnotes

*

This work was supported in part by the National Aeronautics and Space Administration under NASA Grant NGL-14-001-001.

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