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Evidence for downflow following a coronal transientOn 11 September 1973 a peculiar prominence was observed. The prominence displayed strong (approximately 50 km per sec) systematic motions toward and away from the observer. The unusual spectrographic appearance of the prominence might have been due to downflowing material lifted into the corona during an earlier coronal transient.
Document ID
19750059717
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00149920
Authors
Hildner, E. (High Altitude Observatory Boulder, Colo., United States)
Livingston, W. C. (Kitt Peak National Observatory Tucson, Ariz., United States)
Date Acquired
August 8, 2013
Publication Date
June 1, 1975
Publication Information
Publication: Solar Physics
Volume: 42
Subject Category
Solar Physics
Accession Number
75A43789
Funding Number(s)
CONTRACT_GRANT: NAS5-3950
Distribution Limits
Public
Copyright
Other

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