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

doi:10.1117/12.925879

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

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

3 Citations (Scopus)

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.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2012
Subtitle of host publication	Ultraviolet to Gamma Ray
DOIs	https://doi.org/10.1117/12.925879
Publication status	Published - 01-12-2012
Externally published	Yes
Event	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray - Amsterdam, Netherlands Duration: 01-07-2012 → 06-07-2012

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	8443
ISSN (Print)	0277-786X

Other

Other	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Country	Netherlands
City	Amsterdam
Period	01-07-12 → 06-07-12

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.925879

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Ozaki, M., Odaka, H., Sato, T., Yasuda, T., Asai, M., Hiragi, K., Mizuno, T., Mori, H., Terada, Y., & Furuzawa, A. (2012). A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit. In Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray [844356] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8443). https://doi.org/10.1117/12.925879

Ozaki, Masanobu ; Odaka, Hirokazu ; Sato, Tamotsu ; Yasuda, Tetsuya ; Asai, Makoto ; Hiragi, Kazuyoshi ; Mizuno, Tsunefumi ; Mori, Hideyuki ; Terada, Yukikatsu ; Furuzawa, Akihiro. / A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit. Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. 2012. (Proceedings of SPIE - The International Society for Optical Engineering).

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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.",

author = "Masanobu Ozaki and Hirokazu Odaka and Tamotsu Sato and Tetsuya Yasuda and Makoto Asai and Kazuyoshi Hiragi and Tsunefumi Mizuno and Hideyuki Mori and Yukikatsu Terada and Akihiro Furuzawa",

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Ozaki, M, Odaka, H, Sato, T, Yasuda, T, Asai, M, Hiragi, K, Mizuno, T, Mori, H, Terada, Y & Furuzawa, A 2012, A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit. in Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray., 844356, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, Amsterdam, Netherlands, 01-07-12. https://doi.org/10.1117/12.925879

A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit. / Ozaki, Masanobu; Odaka, Hirokazu; Sato, Tamotsu; Yasuda, Tetsuya; Asai, Makoto; Hiragi, Kazuyoshi; Mizuno, Tsunefumi; Mori, Hideyuki; Terada, Yukikatsu; Furuzawa, Akihiro.

Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. 2012. 844356 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8443).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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AU - Ozaki, Masanobu

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AU - Yasuda, Tetsuya

AU - Asai, Makoto

AU - Hiragi, Kazuyoshi

AU - Mizuno, Tsunefumi

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AU - Furuzawa, Akihiro

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AB - 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.

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Ozaki M, Odaka H, Sato T, Yasuda T, Asai M, Hiragi K et al. A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit. In Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. 2012. 844356. (Proceedings of SPIE - The International Society for Optical Engineering). https://doi.org/10.1117/12.925879