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
Author Affiliations +
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
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Gamma radiation

Xenon

Sensors

Electronics

Artificial intelligence

Electrons

Ionization

RELATED CONTENT

Development of high-pressure xenon detectors
Proceedings of SPIE (July 01 1998)
High-pressure xenon gamma-ray large-volume spectrometer
Proceedings of SPIE (October 18 1996)
Neutron-burst timing with sealed tube generators
Proceedings of SPIE (March 03 1995)
Measurement of background 0.1 to 2.0 MeV gamma ray...
Proceedings of SPIE (September 16 1994)

Back to Top