Monte Carlo simulation of atmospheric gamma-ray scattering

Details Monte Carlo simulation of atmospheric gamma-ray scattering Monte Carlo simulation of atmospheric gamma-ray scattering

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..665m&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 665-668 (1984).

Physics

Optics

2

Observation And Data Reduction Techniques, Computer Modeling And Simulation, Atmospheric And Ocean Optics

Scientific paper

The scattering of γ-rays (energy greater than 20 keV) from an astronomical point source in the earth's atmosphere is simulated using Monte Carlo methods. The intensity of scattered γ-rays is estimated as a function of energy, direction, altitude, and geographic location. A few examples of the calculated flux are presented, averaging over direction to simulate the response of a BATSE detector to the scattered radiation.

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