DocumentCode :
3091247
Title :
Continuum background in space-borne gamma-ray detectors
Author :
Evans, L.G. ; Trombka, J.I. ; Starr, R. ; Boynton, W.V. ; Bailey, S.H.
Author_Institution :
Sci. Programs, Comput. Sci. Corp., Lanham-Seabrook, MD, USA
fYear :
1997
fDate :
22-23 Jul 1997
Firstpage :
101
Lastpage :
103
Abstract :
Instrumental backgrounds present a basic limitation to the sensitivity for any gamma-ray detector. This background consists of both discrete lines and a continuum. The discrete background lines are especially important if they occur at the same energies as the lines of interest needed to meet the science objectives of the mission. The continuum background imposes a limit on the signal to noise ratio that can be achieved. Measurements of the gamma-ray continuum background made during the cruise portion of a number of planetary missions are compared. All of these missions used shields to reduce the continuum background. Measurements made during spaceflight can be used to test the effectiveness of different shield designs
Keywords :
astronomical instruments; gamma-ray astronomy; gamma-ray detection; germanium radiation detectors; particle detectors; solid scintillation detectors; 100 keV to 10 MeV; Ge; NaI; continuum background; discrete background lines; instrumental backgrounds; planetary missions; sensitivity; shield design; signal to noise ratio; space-borne gamma-ray detectors; Aircraft manufacture; Extraterrestrial measurements; Gamma ray detection; Gamma ray detectors; Phase detection; Position measurement; Radioactive materials; Solid scintillation detectors; Space vehicles; Testing;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
High Energy Radiation Background in Space, 1997 Conference on the
Conference_Location :
Snowmass, CO
Print_ISBN :
0-7803-4335-2
Type :
conf
DOI :
10.1109/CHERBS.1997.660257
Filename :
660257
Link To Document :
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