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Solar Coronal Magnetic Fields
Published online by Cambridge University Press: 19 July 2016
Abstract
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:
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(1) Comparison with a standard reference magnetic field in the solar corona,
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(2) Possible evidence of substantial small-scale fluctuations of the magnetic field (e.g. in active regions),
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(3) Indication of magnetic fields substantially in excess of the standard distribution (e.g. in limb flare events).
- Type
- 1. The Solar Dynamo
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- Copyright
- Copyright © Kluwer 1993