Ground-based orbit determination for spacecraft formations

S. Sgubini, G. Palmerini
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引用次数: 5

Abstract

Spacecraft formations offer interesting challenges to orbit determination, especially for ground-based tracking. In fact, the limited distances between spacecraft and the possible ambiguity of the observables gathered from the ground have an impact on the solution process. The paper aims to apply the filtering techniques on a refined dynamical model, which can include the main perturbation effects - due to the oblateness of the Earth and, at the lower altitudes, the air drag - on spacecraft trajectories, representing them in series with a remarkably limited number of terms even in eccentric case. The idea is to focus on theoretically expected behavior rather than dealing with an enriched but heavier state including parameters directly related to the perturbing effects. In such a way, it could be possible to obtain a good estimate even with limited spacecraft tracking information. This is an important asset in navigating a formation from the Earth, due to the needed partition of ground station resources among different platforms belonging to the formation, and to the possible ambiguity among the measurements, which further reduce the available data. The specific nature of the dynamic model calls for an estimator with a flexible and “open” architecture, easily allowing for changes and additions in the model itself. Therefore, the estimator selected for testing the approach has been the Unscented Kalman Filter, versatile enough to allow for increasing model accuracy without the need for tedious computation of the Jacobian. This approach is also intended to offer a different way to investigate special perturbed configurations, via the semi-analytical and almost exact representation of the trajectories. In such a perspective, one of the first application, which is shortly outlined in the paper, will be the analysis of spacecraft formations under the J2 effect. In fact, recent studies identified a set of almost periodic relative configurations among the spacecraft. This set (sometimes referred as the special or magical inclination's one) has been recently identified by means of numeric search, and has also received some (partial) explanation. Due to the interest in control effort reduction, it is deemed that a better understanding of this special dynamics, possibly provided by means of a selected modeling approach, can be of some interest
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航天器编队地基轨道测定
航天器编队对轨道确定提出了有趣的挑战,特别是对地面跟踪。事实上,航天器之间的有限距离和从地面收集的观测数据可能存在的模糊性对求解过程产生了影响。本文旨在将滤波技术应用于一个精细的动力学模型,该模型可以包括主要的摄动效应——由于地球的扁率,以及在较低的高度,空气阻力——对航天器的轨迹,即使在偏心的情况下,它们也以非常有限的项数序列表示。这个想法是专注于理论上预期的行为,而不是处理一个丰富但更重的状态,包括与扰动效应直接相关的参数。这样,即使在有限的航天器跟踪信息下,也有可能得到一个很好的估计。由于地面站资源需要在属于地层的不同平台之间进行划分,并且测量结果之间可能存在歧义,这进一步减少了可用数据,因此从地球上导航地层是一项重要的资产。动态模型的特定性质要求估算器具有灵活和“开放”的体系结构,容易地允许在模型本身中进行更改和添加。因此,选择用于测试该方法的估计器是Unscented卡尔曼滤波器,它足够通用,可以在不需要繁琐的雅可比矩阵计算的情况下提高模型精度。这种方法还旨在通过轨迹的半解析和几乎精确的表示,提供一种不同的方法来研究特殊的摄动构型。从这个角度来看,第一个应用之一将是分析J2效应下的航天器编队,这将在论文中简要概述。事实上,最近的研究确定了航天器之间的一组几乎周期性的相对配置。这一组(有时被称为特殊或魔法倾向的一组)最近通过数字搜索被识别出来,并且也得到了一些(部分)解释。由于对减少控制努力的兴趣,人们认为更好地理解这种特殊的动力学(可能通过选定的建模方法提供)可能会引起一些兴趣
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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