タイトル | Zodiacal light dynamics experiment: A wideband imaging Fabry-Perot interferometer |
著者(英) | Young, E.; Nagy, A. F.; Torr, D. G.; Torr, M. R. |
著者所属(英) | Michigan Univ. |
発行日 | 1978-09-01 |
言語 | eng |
内容記述 | The Solar Probe will provide an ideal platform from which to study dynamics of dust particles near the sun by measuring the detailed character of the Fraunhofer structure of the zodiacal light. The suggested instrument is a wideband imaging Fabry-Perot interferometer with state of the art technology in both the optics and the detector. The instrument would function as a high-resolution imaging device providing wavelength resolution of 0.03 A over about a 20 A range. The wideband imaging capability would provide sky maps of the zodiacal light on a despun spacecraft without mechanical scanning. The Solar Probe mission would allow the velocity distribution of the dust to be mapped along most of the trajectory of the spacecraft. |
NASA分類 | SOLAR PHYSICS |
レポートNO | 78N32998 |
権利 | No Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/531416 |
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