Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990spie.1344...82r&link_type=abstract
IN: EUV, X-ray, and Gamma-ray instrumentation for astronomy; Proceedings of the Meeting, San Diego, CA, July 11-13, 1990 (A92-20
Astronomy and Astrophysics
Astronomy
2
Background Radiation, Balloon-Borne Instruments, Fluorescence, Proportional Counters, X Ray Spectra, Computerized Simulation, Gamma Ray Spectra, Monte Carlo Method, Photoabsorption
Scientific paper
The results of an analysis of the background in a fluorescence-gated proportional counter operating over the energy range 3-150 keV are presented. It is found that the dominant background component is that produced by high energy qamma-rays that penetrate the shields and undergo multiple scattering in the detector body, resulting in photoelectric absorption in the detector gas. A careful choice of materials and thickness can move the peak of this emission outside of the detector sensitive range, thereby dramatically reducing the residual background.
Bower Charles R.
Dietz Kurtis L.
Ramsey Brian D.
Weisskopf Martin C.
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