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Possible low energy (E less than keV) nonthermal X-ray eventsA search of the 3- to 30-keV data from the NRL proportional counter detector on the Orbiting Geophysical Observatory-5 (OGO-5) satellite has yielded several events which may be nearly completely nonthermal in the e greater than 3 and less than 10 keV range. In each case an impulsive hard X-ray burst accompained by an impulsive microwave burst was associated with a low energy X-ray burst whose profile was a simple rise and fall. The lack of a two component nature in the low energy range argues that the low energy X-ray flux is due to a single physical mechanism, in this case nonthermal bremsstrahlung from accelerated electrons. However, the spectra and time profiles are quite consistent with a thermal interpretation. Polarization measurements are probably necessary to resolve the physical origin of such bursts.
Document ID
19740013337
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kahler, S. W.
(American Science and Engineering, Inc. Cambridge, MA, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA, Washington High Energy Phenomena on the Sun
Subject Category
Physics, General
Report/Patent Number
NSSDC-ID-68-014A-23-PM
Accession Number
74N21450
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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