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Concerning Magnetic Field Measurements in Prominences Using Zeeman and Hanle Methods

Published online by Cambridge University Press:  12 April 2016

V.S. Bashkirtsev  and
G.P. Mashnich
V.S. Bashkirtsev
Affiliation:
Institute of Solar-Terrestrial Physics, Irkutsk, P.O. Box 4026, Russia
G.P. Mashnich
Affiliation:
Institute of Solar-Terrestrial Physics, Irkutsk, P.O. Box 4026, Russia

Abstract

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A critical review is made of the results of magnetic field measurements in prominences obtained by the Zeeman and Hanle methods. By considering the example of three prominences, some discrepancies between the methods are shown. The authors consider that the magnetic field measurements by the Hanle method inadequately represent the actual magnetic field pattern. To overcome these discrepancies a comparative analysis of magnetic field measurements in prominences by both methods is required.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 90 - 93
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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