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Axial Soft X-ray Brightening Associated with Hα Filaments

Published online by Cambridge University Press:  12 April 2016

Frank C.R. Solberg  and
Alan McAllister
Frank C.R. Solberg
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, Norway
Alan McAllister
Affiliation:
Helio Research, NCAR/HAO, Boulder, CO 80301, USA

Abstract

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We have studied coronal soft X-ray (SXR) arcades around filament channels, as observed with the Yohkoh Soft X-ray Telescope (SXT). We have found about a dozen events (1991–1993). Comparisons with Hα filaments have revealed an association between some SXR structures and filaments. These bright thread-like SXR structures (often) appear to be parallel to and co-spatial with Hα filaments. The SXR structures are occasionally maintained for days, although transient brightening of axial structures is more common.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 171 - 174
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

McAllister, et al. 1992, Publ. Ast. Soc. Jap., 44(5), L205 Google Scholar