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Flare asymmetry as seen in offband H-alpha filtergramsNarrow-band H-alpha filtergrams at + or - 1 A and + or - 2 A from the line center were used to study the asymmetry of flares. Of the 60 flares studied, 92% show red asymmetry while 5% show blue asymmetry. Typically, the filtergrams show a striking dominance of the red wing over the blue wing from onset until late in the decay phase. The difference in intensity of the flare emissions is further augmented by the extensiveness of the emission area in the brighter wing. New kernel-like emissions were often found many minutes after the flare maximum. Spatially, they are displaced from the previous kernels. The late emissions show the same asymmetry as that of the earlier part of the flare.
Document ID
19830047359
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Tang, F.
(Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 11, 2013
Publication Date
February 1, 1983
Publication Information
Publication: Solar Physics
Volume: 83
Subject Category
Solar Physics
Accession Number
83A28577
Funding Number(s)
CONTRACT_GRANT: NOAA-NA-81RA00078
CONTRACT_GRANT: NSF ATM-79-11139
CONTRACT_GRANT: NGL-05-002-034
Distribution Limits
Public
Copyright
Other

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