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Hard X-ray detectors in space are prone to background signals due to theubiquitous cosmic rays and cosmic diffuse background radiation thatcontinuously bombards the satellites which carry the detectors. In general, thebackground intensity depends on the space environment as well as the materialsurrounding the detectors. Understanding the behavior of the background noisein the detector is very important to extract the precise source informationfrom the detector data. In this paper, we carry out Monte Carlo simulationsusing the GEANT-4 toolkit to estimate the prompt background noise measured withthe detectors of the RT-2 Experiment onboard the CORONAS-PHOTON satellite.

Instruments of RT-2 Experiment onboard CORONAS-PHOTON and their test and evaluation IV: Background Simulations using GEANT-4 Toolkit