Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-26T11:41:30.860Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Athay, R.G., Querfeld, C.W., Smartt, R.N., Landi Degl’ Innocenti, E. and Bommier, V. 1983, Solar Phys., 89, 3 CrossRefGoogle Scholar
Bashkirtsev, V.S. & Mashnich, G.P.. 1987, in The Magnetographic Observations of Prominences at the Sayan Observatory, Irkutsk: preprint, 1987, p. 52 Google Scholar
Querfeld, C.W., Smartt, R.N., Bommier, V., Landi Degl’ Innocenti, E. and House, L.L 1985, Solar Phys., 96, 277 Google Scholar
Sahal-Brechot, S., Bommier, V. and Leroy, J.L. 1977, A&A., 59, 223 Google Scholar