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Interpretation of temporal features in an unusual X-ray and microwave burstsObservations are briefly discussed of an event in which microwave and hard X-ray emissions were not correlated in the accepted way. Two impulsive peaks of roughly equal intensity were observed at three different microwave frequencies. The hard X-ray peaks accompanying these, however, differ in intensity by almost two orders of magnitude. Various possible interpretations of this burst are discussed, in the context of familiar models of these emissions. The most likely explanation is that the electron spectrum in the first burst has a break at about 350 keV. General implications for interpretation of X-rays and microwaves are discussed.
Document ID
19860062460
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mackinnon, A. L.
(Glasgow, University United Kingdom)
Costa, J. E. R.
(Glasgow Univ. United Kingdom)
Kaufmann, P.
(Instituto de Pesquisas Espaciais Sao Josedos Campos, Brazil)
Dennis, B. R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
March 1, 1986
Publication Information
Publication: Solar Physics
Volume: 104
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
86A47198
Distribution Limits
Public
Copyright
Other

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