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The structure of the coronal soft X-ray source associated with the dark filament disappearance of 1991 September 28 using the Yohkoh Soft X-ray TelescopeThe structure of the coronal soft X-ray source associated with the dark filament disappearance on September 28, 1991, observed with the Soft X-ray Telescope, is examined as a possible example of the 'eruption-reconnection' model of filament disappearance. The results suggest, however, that this model may not fit. There is a strong possibility that much of the dark filament mass remains in the heated unwinding axial field.
Document ID
19930036506
Document Type
Reprint (Version printed in journal)
Authors
Mcallister, Alan (NASA Marshall Space Flight Center Huntsville, AL, United States)
Uchida, Yutaka (Tokyo Univ. Japan)
Tsuneta, Saku (Tokyo Univ. Mitaka, Japan)
Strong, Keith T. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Acton, Loren W. (Lockheed Research Labs. Palo Alto, CA, United States)
Hiei, Eijiro (National Astronomical Observatory Mitaka, Japan)
Bruner, Marilyn E. (Lockheed Research Labs. Palo Alto, CA, United States)
Watanabe, Takashi (Nagoya Univ. Japan)
Shibata, Kazunari (National Astronomical Observatory Mitaka, Japan)
Date Acquired
August 15, 2013
Publication Date
January 1, 1992
Publication Information
Publication: PASJ: Publications of the Astronomical Society of Japan
Volume: 44
Issue: 5
ISSN: 0004-6264
Subject Category
SOLAR PHYSICS
Funding Number(s)
CONTRACT_GRANT: NAS8-37334
Distribution Limits
Public
Copyright
Other