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A new perspective on solar active regionsA flood of new observations of the solar corona have been made with high spatial resolution, good temporal coverage and resolution, and large linear dynamic range by the Soft X-ray Telescope (SXT) on Yohkoh. These data are changing our fundamental understanding of how solar magnetic fields emerge, interact, and dissipate. This paper reviews some of the results from Yohkoh in the context of earlier results from the Solar Maximum Mission (SMM) and in comjunction with ground-based optical and radio observations.
Document ID
19950064151
Document Type
Reprint (Version printed in journal)
Authors
Strong, K. T. (Lockheed Solar and Astrophysical Laboratory, Palo Alto, CA US, United States)
Bruner, M. E. (Lockheed Solar and Astrophysical Laboratory, Palo Alto, CA US, United States)
Date Acquired
August 17, 2013
Publication Date
January 1, 1996
Publication Information
Publication: Advances in Space Research
Volume: 17
Issue: 5-Apr
ISSN: 0273-1177
Subject Category
SOLAR PHYSICS
Funding Number(s)
CONTRACT_GRANT: NAS8-37334
Distribution Limits
Public
Copyright
Other

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