| 書目名稱 | Theory of Geostationary Satellites | | 編輯 | Chong-Hung Zee | | 視頻video | http://file.papertrans.cn/924/923863/923863.mp4 | | 圖書封面 |  | | 描述 | .Geostationary or equatorial synchronous satellites are a daily reminder of our space efforts during the past two decades. The nightly television satellite weather picture, the intercontinental telecommunications of television transmissions and telephone conversations, and the establishrnent of educational programs in remote regions on Earth are constant reminders of the presence of these satellites. As used here, the term ‘geo- stationary‘ must be taken loosely because, in the long run, the satellites will not remain ‘stationary‘ with respect to an Earth-fixed reference frame. This results from the fact that these satellites, as is true for all satellites, are incessantly subject to perturbations other than the central-body attraction of the Earth. Among the more predominant pertur- bations are: the ellipticity of the Earth‘s equator, the Sun and Moon, and solar radiation pressure. Higher harmonics of the Earth‘s potential and tidal effects also influence satellite motion, but they are of second- order when compared to the predominant perturbations. This volume deals with the theory of geostationary satellites. It consists of seven chapters. Chapter 1 provides a general discussion | | 出版日期 | Book 1989 | | 關(guān)鍵詞 | moon; radiation; satellite; space | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-009-2573-1 | | isbn_softcover | 978-94-010-7662-3 | | isbn_ebook | 978-94-009-2573-1 | | copyright | Springer Science+Business Media Dordrecht 1989 |
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