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Background in X-ray astronomy proportional countersThe authors report the results of an investigation into the nature of background events in proportional counters sensitive to X-ray photons having energy of less than 150 keV. Even with the use of thick shields composed of high-atomic-number material, a significant flux background in the detector's energy region can result from multiple Compton scattering in the mass surrounding the active region of the detector. The importance of the selection of detector components in the reduction of the background by more than an order of magnitude is emphasized. Experimental results are shown to agree qualitatively with Monte Carlo simulations. It is concluded that escape gating is a powerful means of determining the nature of background in flight detectors: the single/pair ratios reveal whether the detected events are charged particles or photons.
Document ID
19910057873
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bower, C. R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Dietz, K. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ramsey, B. D.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Weisskopf, M. C.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 15, 2013
Publication Date
April 1, 1991
Publication Information
Publication: IEEE Transactions on Nuclear Science
Volume: 38
ISSN: 0018-9499
Subject Category
Instrumentation And Photography
Accession Number
91A42496
Distribution Limits
Public
Copyright
Other

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