Paper
22 December 1992 Compressed gaseous xenon gamma-ray detector with high energy resolution
Valery V. Dmitrenko, Aleksey E. Bolotnikov, I. V. Chernycheva, A. M. Galper, V. M. Gratchev, O. N. Kondakova, S. V. Krivov, S. I. Sutchkov, Sergey E. Ulin, Z. M. Uteshev, K. F. Vlasik, Yu. T. Yurkin
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Abstract
A high pressure xenon parallel plate ionization chamber was designed for measurements of cosmic gamma-ray lines. The 3 liter chamber was filled with 0.6 g/cu cm density of xenon, mixed with hydrogen for increasing the drift velocity of the electrons. The noise-subtracted energy resolution was 1.3 percent FWHM at energy 1 MeV. This chamber was installed on the space station 'MIR', currently in orbit and the measurements are being carried out. No energy resolution degradation has been observed for two years, despite the strong irradiation by the Brazil anomaly.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Valery V. Dmitrenko, Aleksey E. Bolotnikov, I. V. Chernycheva, A. M. Galper, V. M. Gratchev, O. N. Kondakova, S. V. Krivov, S. I. Sutchkov, Sergey E. Ulin, Z. M. Uteshev, K. F. Vlasik, and Yu. T. Yurkin "Compressed gaseous xenon gamma-ray detector with high energy resolution", Proc. SPIE 1734, Gamma-Ray Detectors, (22 December 1992); https://doi.org/10.1117/12.138594
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Cited by 2 scholarly publications.
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KEYWORDS
Gamma radiation

Xenon

Sensors

Electronics

Artificial intelligence

Electrons

Ionization

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