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X-ray spectrometer experiment aboard the ISEE-C /Heliocentric/ spacecraftThis experiment is designed to provide continuous coverage of solar flare X-ray bursts and transient cosmic gamma-ray bursts. A proportional counter and a scintillation detector together cover the energy range from 5 to 228 keV with good sensitivity, large dynamic range, and high temporal resolution. This experiment provides data storage capability and good absolute timing so that in conjunction with similar experiments on other spacecraft, accurate source locations can be obtained for cosmic gamma-ray bursts.
Document ID
19780065143
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Anderson, K. A.
(California Univ. Berkeley, CA, United States)
Kane, S. R.
(California Univ. Berkeley, CA, United States)
Primbsch, J. H.
(California Univ. Berkeley, CA, United States)
Weitzmann, R. H.
(California, University Berkeley, Calif., United States)
Evans, W. D.
(California Univ. Berkeley, CA, United States)
Klebesadel, R. W.
(California Univ. Berkeley, CA, United States)
Aiello, W. P.
(California, University Los Alamos Scientific Laboratory, Los Alamos, N. Mex., United States)
Date Acquired
August 9, 2013
Publication Date
July 1, 1978
Publication Information
Publication: IEEE Transactions on Geoscience Electronics
Volume: GE-16
Subject Category
Spacecraft Instrumentation
Accession Number
78A49052
Funding Number(s)
CONTRACT_GRANT: NAS5-22307
Distribution Limits
Public
Copyright
Other

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