利用航天器位置估计精确编队飞行

T. Sanjeeviraja, P. K. Dash
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引用次数: 2

摘要

轨道确定是当前和下一代观测技术的一个视角。作为精密编队飞行需要的高精度定轨系统(HAODS)的一部分,需要确定航天器在轨道上的位置和速度。考虑空间物体连续三次的三个地心位置向量。被观测物体的角度位置及其在给定历元的时间导数用于分析。改进的角度观测有助于近地点高度和时间的确定。改进了传统的高精度定轨角度观测。计算结果给出了航天器在指定轨道元上的初始、最终位置和速度矢量,为更详细地分析轨道周期提供了一种模式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Estimation of precision formation flying using position of the spacecraft
Orbit determination is a perspective of the current and next generation observational technique. As a part of the precision formation flying need's High Accuracy Orbit Determination System (HAODS), it is required to find the position and velocity of spacecraft on the orbit. Three geocentric position vectors of a space object at a three successive times are considered. The angular positions of the observed body and their time derivatives at a given epoch are used for analysis. The improved angular observation is aided in the determination of perigee altitude and the time. It improved angular observations with traditional high accuracy in orbit determination. The results presented the initial and final position and velocity vector of the spacecraft on specified orbital elements and provide a mode for more detailed analysis of the orbital period.
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