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Correlation of hard X-ray and type III bursts in solar flaresCorrelations between X-ray and type 3 radio emission of solar bursts are described through a bivariate distribution function. Procedures for determining the form of this distribution are described. A model is constructed to explain the correlation between the X-ray spectral index and the ratio of X-ray to radio intensities. Implications of the model are discussed. Previously announced in STAR as N82-32243
Document ID
19830066497
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00151167
Authors
Petrosian, V. (Stanford Univ. CA, United States)
Leach, J. (Stanford University Stanford, CA, United States)
Date Acquired
August 11, 2013
Publication Date
August 1, 1983
Publication Information
Publication: Solar Physics
Volume: 87
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
83A47715
Funding Number(s)
CONTRACT_GRANT: NSG-7092
CONTRACT_GRANT: NSF ATM-81-16989
Distribution Limits
Public
Copyright
Other

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