双旋卫星姿态采集中两种磁阻尼规律的比较

IF 0.2
M. Ovchinnikov, D. Roldugin
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引用次数: 0

摘要

考虑了卫星姿态获取阶段的双旋运动。从任意旋转状态出发,卫星最终的角动量应与轨道法线对齐。卫星配备了磁致力矩器来提供角速度阻尼。比较了两种控制策略,即简单指数阻尼和由经典滑动控制实现产生的“加权”阻尼。分析了控制系统随卫星惯性矩变化的时间响应。简单阻尼被证明可以在低控制权限下提供更好的效果,即使对于明显拉长的卫星。用特征指数近似的解析解证明了这一结果。数值模拟结果表明,加权阻尼对显著控制权限具有较好的控制效果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparison of two magnetic damping laws for the attitude acquisition of a dual spin satellite
Dual spin satellite motion in the attitude acquisition phase is considered. Starting from the arbitrary rotation state, the satellite should end up with its angular momentum aligned with the orbit normal. The satellite is equipped with magnetorquers that provide the angular velocity damping. Two control strategies are compared, that is the simple exponential damping and 'weighted' damping arising from the classical sliding control implementation. The time response of the control system depending on the satellite inertia moments is analysed. Simple damping is proven to provide better results for the low control authority even for the significantly elongated satellite. This result is proved with the analytical solution for the characteristic exponents approximations. Weighted damping is shown to provide better results for significant control authority through numerical simulation.
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