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Combined analysis of soft and hard X-ray spectra from flaresAn attempt is made to develop a self-consistent model which accounts for the line and continuum data generated by the three X-ray imaging instruments on the SMM satellite. The intensities measured covered the 4-500 kV energy range. The model is based on a differential emission measure and electron beam parameters and is used to predict absolute signals detected by the 15 channels of the SMM sensors. Consideration is given to the thermal contribution, instrumental characteristics, thin target excitation and thick target bremsstrahlung. In comparison with data from a flare event on June 29, 1980, model predictions provide a good fit, including the identification of hard electrons with a 5.3 index during the impulsive phase.
Document ID
19850046185
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gabriel, A. H.
(Science Research Council Chilton, United Kingdom)
Sherman, J. C.
(Science and Engineering Research Council, Rutherford Appleton Laboratory, Didcot Oxon, United Kingdom)
Bely-Dubau, E.
(Nice Observatoire, Nice, France)
Orwig, L. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Schrijver, J.
(Laboratorium voor Ruimteonderzoek Utrecht, Netherlands)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Advances in Space Research
Volume: 4
Issue: 7, 19
ISSN: 0273-1177
Subject Category
Solar Physics
Accession Number
85A28336
Distribution Limits
Public
Copyright
Other

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