摘要
共面编队飞行的卫星星座的相对运动轨迹是一个椭圆,但卫星由于受摄动力的影响,其椭圆队形会发生变化。提出了一个简单而又节约燃料的队形保持控制方案,即在Hill轨道坐标系中,通过测量x轴和z轴,利用小推力喷气发动机进行控制,消除椭圆中心的相位漂移和各卫星轨道的不共面。
The figure of the relative kinematical track of the formation flying will change which is in an ellipse because of the disturbing force from which the satellites suffer. A simple way of control is developed that saves the fuel, that is, in Hill orbital coordinates, through the measurement of x-axis and z-axis, the control of the small jet engine will eliminate the phase excursion of the center of the ellipse and the non-coplanarity of the orbit of satellites.
出处
《国防科技大学学报》
EI
CAS
CSCD
北大核心
2004年第3期24-28,共5页
Journal of National University of Defense Technology
关键词
共面编队飞行
星座
轨道控制
satellites formation flying
constellations
orbital control