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 | |
| Publication status | Published - 01-12-2012 |
| 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 |
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All Science Journal Classification (ASJC) codes
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering
Cite this
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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
TY - GEN
T1 - A Monte Carlo simulation framework to study ASTRO-H in-orbit radiation and detector responses based on Geant4 toolkit
AU - Ozaki, Masanobu
AU - Odaka, Hirokazu
AU - Sato, Tamotsu
AU - Yasuda, Tetsuya
AU - Asai, Makoto
AU - Hiragi, Kazuyoshi
AU - Mizuno, Tsunefumi
AU - Mori, Hideyuki
AU - Terada, Yukikatsu
AU - Furuzawa, Akihiro
PY - 2012/12/1
Y1 - 2012/12/1
N2 - 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.
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.
UR - http://www.scopus.com/inward/record.url?scp=84871743355&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84871743355&partnerID=8YFLogxK
U2 - 10.1117/12.925879
DO - 10.1117/12.925879
M3 - Conference contribution
AN - SCOPUS:84871743355
SN - 9780819491442
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2012
ER -