| タイトル | High energy gamma ray results from the second small astronomy satellite |
| 本文（外部サイト） | http://hdl.handle.net/2060/19740027105 |
| 著者（英） | Kniffen, D. A.; Fichtel, C. E.; Bignami, G. F.; Oezel, M. F.; Thompson, D. J.; Hartman, R. C.; Oegelman, H.; Tuemer, T. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1974-10-01 |
| 言語 | eng |
| 内容記述 | A high energy (35 MeV) gamma ray telescope employing a thirty-two level magnetic core spark chamber system was flown on SAS 2. The high energy galactic gamma radiation is observed to dominate over the general diffuse radiation along the entire galactic plane, and when examined in detail, the longitudinal and latitudinal distribution seem generally correlated with galactic structural features, particularly with arm segments. The general high energy gamma radiation from the galactic plane, explained on the basis of its angular distribution and magnitude, probably results primarily from cosmic ray interactions with interstellar matter. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 74N35218
X-662-74-304
NASA-TM-X-70761 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/192519 |
|
