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Solar Coronal Magnetic Fields

Published online by Cambridge University Press:  19 July 2016

J. Hildebrandt ,
B. Kliem  and
A. Krüger
J. Hildebrandt
Affiliation:
Astrophysical Institute Potsdam, Germany
B. Kliem
Affiliation:
Astrophysical Institute Potsdam, Germany
A. Krüger
Affiliation:
Astrophysical Institute Potsdam, Germany

Abstract

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A short compilation of various radio methods of the determination of magnetic fields in the solar corona is given which, completed by observations in other spectral ranges (e.g. the optical and X-ray ranges), results in a complex picture of the magnetic field. Some topics of interest are the following:

  1. (1) Comparison with a standard reference magnetic field in the solar corona,

  2. (2) Possible evidence of substantial small-scale fluctuations of the magnetic field (e.g. in active regions),

  3. (3) Indication of magnetic fields substantially in excess of the standard distribution (e.g. in limb flare events).

Type
1. The Solar Dynamo
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 59 - 61
Copyright
Copyright © Kluwer 1993 

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