Particle transport simulation for spaceborne, NaI gamma-ray spectrometers

Details Particle transport simulation for spaceborne, NaI gamma-ray spectrometers Particle transport simulation for spaceborne, NaI gamma-ray spectrometers

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...9013292d&link_type=abstract

Presented at the IEEE Nuclear and Space Radiation Effects Conference, Portland, OR, 11-15 Jul. 1988

Astronomy and Astrophysics

Astronomy

Computerized Simulation, Gamma Ray Observatory, Gamma Ray Spectrometers, Radiation Transport, Sodium Iodides, Background Radiation, Monte Carlo Method, Particle Motion, Protons, Spaceborne Astronomy

Scientific paper

Spaceborne gamma-ray spectrometers sensitivity is investigated. Monte Carlo transport codes are employed to simulate particle transport of cosmic rays and inner-belt protons in representations of the gamma-ray observatory spacecraft and the oriented scintillation spectrometer experiment. Results are used to quantify the contributions to the radioactive background, assess shielding options and examine the effect of detector and spacecraft orientation in anisotropic trapped proton fluxes.

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