星座
卫星
地面轨道
计算机科学
轨道(动力学)
卫星星座
视野
交叉口(航空)
摄动(天文学)
算法
经度
不变(物理)
领域(数学)
大地测量学
拓扑(电路)
数学
物理
纬度
航空航天工程
地理
计算机视觉
纯数学
组合数学
天文
工程类
数学物理
地球静止轨道
作者
Shengzhou Bai,Yujin Zhang,Yiping Jiang,Yuhan Chen
标识
DOI:10.1109/taes.2023.3240675
摘要
This article proposes a geometric-based method of the ground-point visibility from a satellite or satellite constellation in elliptical orbit considering the J 2 perturbation. First, the field-element equations describing the relationship between the elliptical satellite orbit, field parameters, and ground point are introduced and can be solved semi-analytically. Also, using a 2-D map composed of the mean argument of latitude and geographic longitude of the ascending node, the problem of calculating visible intervals is transformed into a simple intersection problem of a group of parallel lines and a time-invariant region generated by the field-element equations. Furthermore, based on the geometric relationship between any two satellites, the relative field mapping and constellation field mapping are described, which can simplify the multisatellite coverage problem to a single-satellite coverage problem and can be used to obtain the coverage performance of the constellation analytically and rapidly for the target. The simulation results demonstrate that the proposed method is rapid, efficient, intuitive, and accurate, suggesting its wide applications in constellation studies.
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