| 地球引力场对卫星有摄运动的一种计算方法 |
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| 引用本文： | 郑文虎. 地球引力场对卫星有摄运动的一种计算方法[J]. 应用数学和力学, 1997, 18(2): 153-160 |
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| 作者姓名： | 郑文虎 |
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| 作者单位： | 西昌师范高等专科学校物理系, 四川西昌 615022 |
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| 摘 要： | 本文应用Delaunay变量,从理论力学的哈密顿方程出发,通过正则变换求解了地球引力摄动对卫星运动轨道的影响,导出卫星位置和速度随时间的变化关系.
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| 关 键 词： | 地球引力场 哈密顿方程 摄动 正则变换 |
| 收稿时间： | 1995-10-09 |
A Calculation Method to the Perturbation of a Satellite Caused by the Gravitation Field of the Earth |
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| Zheng Wenhu. A Calculation Method to the Perturbation of a Satellite Caused by the Gravitation Field of the Earth[J]. Applied Mathematics and Mechanics, 1997, 18(2): 153-160 |
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| Authors: | Zheng Wenhu |
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| Affiliation: | Department of Physics, Xichang Teacher's College, Xichang, Sichuan 615022, P. R. China |
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| Abstract: | In this paper, with the application of the Delauney variables, according to the Hamilton equations, the influence on the perturbation of a satellite exerted by the gravitational force of the earth through canonical transformation has been found out. As a result, the equation about how the position and velocity of the satellite vary with time is deduced. |
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| Keywords: | gravitation field Hamilton equation perturbation canonical transformation. |
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