Configuration Uncertainty Propagation of Geocentric Interferometric Constellation with Respect to Orbital Element Errors

F. Jia, Xiangyu Li, Xingyu Zhou, D. Qiao
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Abstract

The interferometric constellations are widely applied to high-precision measurement in space, such as space gravitational waves detection. Uncertain propagation study of constellations can provide guidance for configuration design, but highly nonlinear dynamics and large evolution time make it very difficult. This paper aims at the uncertainty propagation of the geocentric interferometric constellations under the action of complex conservative forces. First, the configuration parameters of a constellation are introduced. The magnitudes of the conservative perturbations at different orbital altitudes are analyzed, including the third body perturbations from the Moon, the Sun and the Earth's non-spherical perturbation. Secondly, the initial state of the constellation is represented by the set of orbital elements of each spacecraft. The deviations of the orbital elements are separately applied to the initial configurations of different orientations and sizes to study the configuration uncertainty propagations. It is found that the accumulation of phase deviation is the major factor leading to the configuration deformation. The uncertainty magnitude of the constellation is inversely related to the configurational size. Besides, the configuration of the constellations, whose orbital period is resonated with the Moon, should be avoided in the mission design.
考虑轨道元误差的地心干涉星座构型不确定度传播
干涉星座被广泛应用于空间高精度测量,如空间引力波探测。星座的不确定性传播研究可以为构型设计提供指导,但高度非线性的动力学特性和大的演化时间使得设计难度很大。本文研究了地心干涉星座在复保守力作用下的不确定性传播。首先,介绍了星座的构型参数。分析了不同轨道高度的保守扰动的大小,包括来自月球、太阳和地球的非球面扰动的第三体扰动。其次,用各航天器的轨道元集合来表示星座的初始状态。将轨道元的偏差分别应用于不同方向和尺寸的初始构型,研究构型不确定性的传播。研究发现,相位偏差的累积是导致结构变形的主要因素。星座的不确定度大小与构型尺寸成反比。此外,在任务设计中应避免星座的配置与月球的轨道周期产生共振。
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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