【摘 要】
：
该文基于L aw den方程分别对圆参考轨道和椭圆参考轨道的卫星理想编队队形设计进行了研究。对于圆参考轨道,通过引入相角概念,简化了多星编队队形设计,并通过理论分析和算例
【机 构】
：
清华大学航天航空学院,清华大学航天航空学院,清华大学航天航空学院 北京100084,北京100084,北京100084
论文部分内容阅读
该文基于L aw den方程分别对圆参考轨道和椭圆参考轨道的卫星理想编队队形设计进行了研究。对于圆参考轨道,通过引入相角概念,简化了多星编队队形设计,并通过理论分析和算例仿真说明:编队队形与初始真近点角的选择无关,且有多组从星运动参数组合满足队形设计要求。对于椭圆参考轨道编队,编队队形的变化与主星的轨道偏心率及编队初始真近点角的选择密切相关,且满足队形要求的从星运动参数组合是惟一的。
Based on the L aw den equation, this paper studies the satellite ideal formation formation design of circular or elliptical reference orbit. For the circular reference orbit, by introducing the concept of phase angle, the formation design of multi-star formation is simplified. Theoretical analysis and case simulation show that formation formation has nothing to do with the selection of the initial true near-point angle, Combination of parameters to meet the requirements of the formation design. For elliptical reference orbital formation, formation formation formation is closely related to the orbital eccentricity of the main star and the formation of the initial true and near angles, and the combination of the star motion parameters satisfying the formation requirements is unique.
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