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首页> 外文期刊>Acta astronautica >Quaternion-based adaptive attitude control of asteroid-orbiting spacecraft via immersion and invariance
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Quaternion-based adaptive attitude control of asteroid-orbiting spacecraft via immersion and invariance

机译:基于四元数的沉浸和不变性的小行星轨道航天器自适应姿态控制

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摘要

The design of an attitude control system for an asteroid-orbiting satellite via immersion and invariance is the subject of this paper. It is assumed that the asteroid is rotating with a constant rate, and that the inertia parameters of the satellite and the coefficients in the spherical harmonic gravitational potential of the asteroid are not known. The objective is to regulate the quaternion trajectory of the satellite orbiting in an equatorial orbit. Based on the immersion and invariance (I&I) theory, a noncertainty-equivalence adaptive (NCEA) attitude control law is derived. For the design, a backstepping design process involving two steps is used, and filtered signals are constructed to overcome the difficulty in solving certain matrix inequalities of the I&I methodology. The control law includes a stabilizer and an identifier - designed separately. Unlike the classical certainty-equivalence adaptive (CEA) systems, here the estimated parameters include not only the signals obtained from an integral type update law, but also judiciously chosen nonlinear algebraic signals that yield stronger stability properties. By the Lyapunov stability analysis, it is shown that the quaternion trajectories of the disturbance input-free closed-loop system asymptotically converge to the equilibrium point. The control law is effective in regulating the attitude to the equilibrium point with minimal rotation of spacecraft. Also, for the model with disturbance input, uniform ultimate boundedness of system trajectories is established. Simulation results for the attitude control of spacecraft in orbit around asteroid 433 Eros are presented for illustration. These results show that the spacecraft achieves nadir pointing attitude despite uncertainties in the system dynamics.
机译:通过沉浸和不变性设计小行星轨道卫星的姿态控制系统是本文的主题。假定小行星以恒定的速率旋转,并且卫星的惯性参数和小行星的球谐重力引力的系数未知。目的是调节在赤道轨道上运行的卫星的四元数轨迹。基于沉浸和不变性(I&I)理论,推导了不确定性等价自适应(NCEA)姿态控制定律。对于设计,使用了包含两步的后推设计过程,并构造了滤波信号以克服解决I&I方法的某些矩阵不等式的困难。控制律包括稳定器和标识符-分别设计。与经典的等价性自适应(CEA)系统不同,这里的估计参数不仅包括从整数类型更新定律获得的信号,而且还包括明智选择的产生更强稳定性的非线性代数信号。通过李雅普诺夫稳定性分析,表明无扰动闭环系统的四元数轨迹渐近收敛于平衡点。控制定律有效地以最小的航天器旋转来调节对平衡点的姿态。此外,对于具有干扰输入的模型,建立了系统轨迹的统一最终有界性。为了说明,提出了围绕小行星433 Eros进行轨道航天器姿态控制的模拟结果。这些结果表明,尽管系统动力学存在不确定性,但航天器仍达到了最低点的姿态。

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