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A simple solar microwave burst observed with high spectral resolutionA small flare that occurred on February 3, 1986 which was dominated by a single homogeneous source is analyzed. The theory of microwave emission from homogeneous sources was used to trace the evolution of the burst. The spectral profile indicates a thermal origin. It was found that the source expanded with time during the burst.
Document ID
19890049501
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/167366
Authors
Gary, Dale E. (California Inst. of Tech. Pasadena, CA, United States)
Hurford, G. J. (Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
April 15, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 339
ISSN: 0004-637X
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0004-637X
Accession Number
89A36872
Funding Number(s)
CONTRACT_GRANT: NSF AST-87-02682
CONTRACT_GRANT: F19628-86-K-0017
CONTRACT_GRANT: NSF ATM-86-10330
CONTRACT_GRANT: NAG5-946
Distribution Limits
Public
Copyright
Other

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