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Monte Carlo simulation of a new gamma ray telescopeA new Monte Carlo code has been written to simulate the response of the new University of California double scatter gamma ray telescope. This package of modular software routines, written in VAX FORTRAN 77 simulates the detection of 0.1 to 35 MeV gamma rays. The new telescope is flown from high altitude balloons to measure medium energy gamma radiation from astronomical sources. This paper presents (1) the basic physics methods in the code, and (2) the predicted response functions of the telescope. Gamma ray processes include Compton scattering, pair production and photoelectric absorption in plastic scintillator, NaI(Tl) and aluminum. Electron transport processes include ionization energy loss, multiple scattering, production of bremsstrahlung photons and positron annihilation.
Document ID
19850039629
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Simone, J.
(California State University Los Angeles, CA, United States)
Oneill, T.
(California State Univ. Los Angeles, CA, United States)
Tumer, O. T.
(California State Univ. Los Angeles, CA, United States)
Zych, A. D.
(California, University Riverside, CA, United States)
Date Acquired
August 12, 2013
Publication Date
February 1, 1985
Publication Information
Publication: IEEE Transactions on Nuclear Science
Volume: NS-32
ISSN: 0018-9499
Subject Category
Astronomy
Accession Number
85A21780
Funding Number(s)
CONTRACT_GRANT: NGR-05-008-022
Distribution Limits
Public
Copyright
Other

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