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A mercuric detector system for X-ray astronomy. 2. Results from flight tests of a balloon borne instrumentTo establish the expected sensitivity of a new hard X-ray telescope design, an experiment was conducted to measure the background counting rate at balloon altitudes (40 km) of mercuric iodide, a room temperature solid state X-ray detector. The prototype detector consisted of two thin mercuric iodide (HgI2) detectors surrounded by a large bismuth germanate (Bi4Ge3O12) scintillator operated in anticoincidence. The bismuth germanate shield vetoed most of the background counting rate induced by atmospheric gamma-rays, neutrons and cosmic rays. A balloon-borne gondola containing a prototype detector assembly was designed, constructed and flown twice in the spring of 1982 from Palestine, Texas. The second flight of this instrument established a differential background counting rate of 4.2 O.7 x 10-5 counts/sec cm keV over the energy range of 40 to 80 keV. This measurement was within 50% of the predicted value. The measured rate is approx 5 times lower than previously achieved in shielded NaI/CsI or Ge systems operating in the same energy range. The prediction was based on a Monte Carlo simulation of the detector assembly in the radiation environment at float altitude.
Document ID
19840008027
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Vallerga, J.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Vanderspek, R. K.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Ricker, G. R.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Date Acquired
September 4, 2013
Publication Date
January 1, 1982
Subject Category
Astronomy
Report/Patent Number
NASA-CR-175329
NAS 1.26:175329
Accession Number
84N16095
Funding Number(s)
CONTRACT_GRANT: NSG-7339
CONTRACT_GRANT: NAGW-14
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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