Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l.205m&link_type=abstract
PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 5, p. L205-L210.
Astronomy and Astrophysics
Astronomy
46
Dark Matter, Solar Corona, Solar Prominences, Solar X-Rays, Spaceborne Astronomy, H Alpha Line, Japanese Spacecraft, X Ray Telescopes
Scientific paper
The 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.
Acton Loren W.
Bruner Marilyn E.
Hiei Eijiro
McAllister Alan
Shibata Kazunari
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