Abstract
Using Geant4 Monte Carlo simulation code, background gamma rays for Gamma Ray Spectrometer onboard SELENE were estimated. Gamma ray emissions from the spacecraft body by leakage neutrons from the Moon and GCR protons were calculated as well as ones from the Moon. It is found that a BGO background reduction system works so well that the background gamma rays produced from the spacecraft body is small in the energy spectrum to be observed by the spectrometer in SELENE.
| Original language | English |
|---|---|
| Title of host publication | Astroparticle, Particle and Space Physics, Detectors and Medical Physics Applications - Proceedings of the 9th Conference |
| Pages | 490-494 |
| Number of pages | 5 |
| Publication status | Published - 2006 |
| Event | International Conference on Advanced Technology and Particle Physics, ICATPP 2005 - Como Duration: 2005 Oct 17 → 2005 Oct 21 |
Other
| Other | International Conference on Advanced Technology and Particle Physics, ICATPP 2005 |
|---|---|
| City | Como |
| Period | 05/10/17 → 05/10/21 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Nuclear and High Energy Physics
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Okudaira, O., Yamashita, N., Hasebe, N., Miyachi, M., Miyajima, M., Hareyama, M., Sakurai, K., Yamamoto, H., Kobayashi, M. N., Shibamura, E., & Hiramoto, T. (2006). GEANT4 Monte Carlo simulation to estimate gamma-ray emissions from lunar surface and selene spacecraft. In Astroparticle, Particle and Space Physics, Detectors and Medical Physics Applications - Proceedings of the 9th Conference (pp. 490-494)