DocumentCode :
3084036
Title :
AXAF detector backgrounds produced by cosmic ray protons
Author :
Armstrong, T.W. ; Colborn, B.L. ; Dietz, K.L. ; O´Dell, S.L. ; Weisskopf, M.C.
Author_Institution :
Sci. Applications Int. Corp., Prospect, TN, USA
fYear :
1997
fDate :
22-23 Jul 1997
Firstpage :
3
Lastpage :
8
Abstract :
X-ray detector backgrounds expected for the planned AXAF mission due to the galactic cosmic ray (GCR) proton environment have been determined by detailed Monte Carlo simulations. The predicted GCR-induced prompt and activation backgrounds are about 0.03 and 0.02 counts/cm2-s, respectively which are small compared to signal strengths expected for planned AXAF observation scenarios
Keywords :
X-ray apparatus; X-ray astronomy; X-ray detection; astronomical instruments; astronomical telescopes; cosmic ray protons; cosmic rays; AXAF; Advanced X-ray Astrophysics Facility; Monte Carlo simulation; X-ray detector background; X-ray telescope; astronomical telescope; cosmic ray proton; cosmic rays; detector noise; galactic cosmic ray; Data analysis; Libraries; Monte Carlo methods; Neutrons; Numerical simulation; Production; Protons; Radioactive materials; Solid modeling; X-ray detectors;
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.1997.660219
Filename :
660219
Link To Document :
بازگشت