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Mass motions associated with solar flaresMass motions are a principal means by which components of solar flares can be distinguished. Typical patterns of mass motions in H-alpha are described for chromospheric flare ribbons, remote chromospheric flare patches, flare loops, flaring arches, surges, erupting filaments and some expanding coronal features. Interrelationships between these phenomena are discussed and illustrations of each are presented.
Document ID
19900027760
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00161697
Authors
Martin, Sara F. (Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Solar Physics
Volume: 121
Issue: 2-Jan
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
90A14815
Funding Number(s)
CONTRACT_GRANT: NSF ATM-85-13577
CONTRACT_GRANT: NGL-05-002-034
CONTRACT_GRANT: AF-AFOSR-87-0023
Distribution Limits
Public
Copyright
Other

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