Paper
17 September 2012 A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit
Masanobu Ozaki, Hirokazu Odaka, Tamotsu Sato, Tetsuya Yasuda, Makoto Asai, Kazuyoshi Hiragi, Tsunefumi Mizuno, Hideyuki Mori, Yukikatsu Terada, Akihiro Furuzawa
Author Affiliations +
Abstract
We are developing an ASTRO-H data analysis framework with the Geant4-based Monte Carlo simulation core, and numerical models of the on-orbit environmental radiation and full-satellite mass structure. The framework uses not only Geant4 but also a traditional X-ray mirror ray-tracing simulator, and a file format compatible with the SimX simulator for input and output of celestial body information. The data exchange between the framework and the external software is based on FITS files, which makes it easy to record and trace the internal steps of the whole simulation framework.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Masanobu Ozaki, Hirokazu Odaka, Tamotsu Sato, Tetsuya Yasuda, Makoto Asai, Kazuyoshi Hiragi, Tsunefumi Mizuno, Hideyuki Mori, Yukikatsu Terada, and Akihiro Furuzawa "A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit", Proc. SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, 844356 (17 September 2012); https://doi.org/10.1117/12.925879
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Cited by 3 scholarly publications.
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KEYWORDS
Monte Carlo methods

Sensors

X-rays

Mirrors

Particles

Satellites

X-ray imaging

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