周期轨道和姿态变化的King-Hele轨道理论

V. Ray, D. Scheeres
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引用次数: 0

摘要

King-Hele提出的大气中卫星轨道解析理论在简化的假设条件下精确逼近数值积分,至今仍广泛应用于卫星任务设计。在过去的60年里,对这一理论的修正弥补了它的许多弱点。然而,在对原始理论的所有后续修改中,一直保留了恒定阻力系数的假设。阻力系数是一个动态参数,它支配着大气和卫星之间的物理相互作用,并取决于环境因素和卫星特定因素。在这项工作中,阻力系数的傅立叶级数展开模型被纳入原始的King-Hele理论中,以捕获平均积分中阻力系数的时间变化。通过仿真验证了改进后的理论,表明与原始King-Hele公式相比,在近似数值结果方面取得了改进。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
King-Hele orbit theory for periodic orbit and attitude variations
The analytical theory of satellite orbits in an atmosphere developed by King-Hele remains widely in use for satellite mission design because of its accurate approximation to numerical integration under simplifying assumptions. Over the course of six decades, modifications to the theory have addressed many of its weaknesses. However, in all subsequent modifications of the original theory, the assumption of a constant drag-coefficient has been retained. The drag-coefficient is a dynamic parameter that governs the physical interaction between the atmosphere and the satellite and depends on ambient as well as satellite specific factors. In this work, Fourier series expansion models of the drag-coefficient are incorporated in the original King-Hele theory to capture time-variations of the drag-coefficient in averaging integrals. The modified theory is validated through simulations that demonstrate the attained improvements in approximating numerical results over the original King-Hele formulation.
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