抜粋
CALET is a detector planned to be on board ISS to investigate high energy universe by observing high energy gamma-rays, electrons and other cosmic ray. It is now in the phase A/B study period of the JAXA program. The performance of CALET was studied earlier[1] but the design structure (mainly its size) has been changed since that time. We have been performing new M.C simulations corresponding to the new structure to evaluate its basic performance. This is to report some of the new results.
| 元の言語 | English |
|---|---|
| ページ | 1433-1436 |
| ページ数 | 4 |
| 出版物ステータス | Published - 2007 1 1 |
| イベント | 30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico 継続期間: 2007 7 3 → 2007 7 11 |
Conference
| Conference | 30th International Cosmic Ray Conference, ICRC 2007 |
|---|---|
| 国 | Mexico |
| 市 | Merida, Yucatan |
| 期間 | 07/7/3 → 07/7/11 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics
フィンガープリント Expected performance of CALET' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。
これを引用
Kasahara, K., Torii, S., Shimizu, Y., Akaike, Y., Taira, K., Yoshida, K., & Watanabe, I. (2007). Expected performance of CALET. 1433-1436. 論文発表場所 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.