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Organization of Uniform Dispersal for Group of Small Satellites After Their Separation and Acceptable Spread at Stages of Their Further Approaches

机译:小卫星群在进一步发展阶段分离和可接受扩展后的均匀分散组织

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Mutual-relative motion of satellites constellation after their placing into initial orbit is characterized the satellites reiterated approaches to minimal distances. Determined separation conditions for each satellite pair in constellation, which realization leads to minimal satellites approaches. It was sustained, that distances between satellites can reach extreme minimal values due to minor angular deviations of orbit planes and always occurring flight altitudes long-period oscillations. Received analytical relations for estimation of angular deviations and distances between satellites orbit planes at the phases of periodical approaches. It was approved that in some vicinity of orbit numbers can occur following almost simultaneously: small differences of angular distances from the equator for any satellite pair in constellation; minimal angular deviations of satellites orbit planes (in general they have different precession after separation of different directions and with various velocities). Analytical relationships were numerically confirmed with using software for satellites movement prediction at the phases of their approaches to the minimum distances. The area of satellites separation parameters was built, with its implementation in a small vicinity of flight orbits the satellites approach to distances less than 100 m. The minimum distance in the specified area according to the single calculations is ~10 m.
机译:卫星星座进入初始轨道后的相互相对运动是卫星重申最小距离的方法的特征。确定星座图中每个卫星对的分离条件,这种实现导致最少的卫星进近。可以肯定的是,由于轨道平面的微小角度偏差以及始终发生的飞行高度长期振荡,卫星之间的距离可以达到极小值。在周期性进场阶段,用于估计卫星轨道平面之间的角度偏差和距离的分析关系。公认的是,在几乎同时发生的轨道数附近可能会发生变化:星座中任何一对卫星到赤道的角距离的微小差异;卫星轨道平面的最小角度偏差(通常,它们在分离不同方向和速度后具有不同的进动)。使用软件对卫星运动进行预测,并在接近最小距离的阶段对这些分析关系进行了数值确认。建立了卫星分离参数区域,并在飞行轨道的小范围内实施了卫星进近距离小于100 m的方法。根据一次计算,指定区域内的最小距离为〜10 m。

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