| タイトル | Inflight Performance of the SDO Fine Pointing Science Mode |
| 本文（外部サイト） | http://hdl.handle.net/2060/20170001432 |
| 著者（英） | Starin, Scott R.; Mason, Paul; O'Donnell, James; Vess, Melissa F.; Halverson, Julie |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2017-02-03 |
| 言語 | eng |
| 内容記述 | The Solar Dynamics Observatory (SDO) was successfully launched and deployed from its Atlas V launch vehicle on February 11, 2010. Three months later, on May 14, 2010, the fully commissioned heliophysics laboratory was handed over to Space Systems Mission Operations to begin its science mission. SDO is an Explorer-class mission now operating in a geosynchronous orbit, sending data 24 hours per day to a dedicated ground station in White Sands, New Mexico. It carries a suite of instruments designed to observe the Sun in multiple wavelengths at unprecedented resolution. The Atmospheric Imaging Assembly (AIA) includes four telescopes with 4096x4096 focal plane CCDs that can image the full solar disk in seven extreme ultraviolet and three ultraviolet-visible wavelengths. The Extreme Ultraviolet Variability Experiment (EVE) collects time-correlated data on the activity of the Sun's corona. The Helioseismic and Magnetic Imager (HMI) enables study of pressure waves moving through the body of the Sun. |
| NASA分類 | Spacecraft Design, Testing and Performance |
| レポートNO | GSFC-E-DAA-TN38940 |
| 権利 | No Copyright |
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