タイトル | Solar response of the BATSE instrument on the gamma-ray observatory |
本文(外部サイト) | http://hdl.handle.net/2060/19890006502 |
著者(英) | Meegan, C. A.; Teegarden, B.; Paciesas, W.; Hudson, Hugh; Parnell, T. A.; Wilson, R. B.; Fishman, G. J.; Schaefer, B.; Cline, T.; Matteson, J. L. |
著者所属(英) | NASA Marshall Space Flight Center |
発行日 | 1988-11-01 |
言語 | eng |
内容記述 | The Burst and Transient Source Experiment (BATSE) on board the gamma ray observatory (GRO) aims at comprehensive observations of time profiles, spectra, and locations of high-energy transient sources. The mysterious cosmic gamma ray bursts provided the main motivation for the observations, but BATSE will make excellent observations of many classes of sources, and in particular solar flares. The solar response of BATSE, as inferred from its design parameters, is analyzed for two purposes: the optimization of the solar observations themselves, and the characterization of the solar effects on ordinary nonsolar observations. |
NASA分類 | SOLAR PHYSICS |
レポートNO | 89N15873 |
権利 | No Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/143720 |
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