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Active nutation damping of asymmetric spinning spacecraft: A Lyapunov design approach.

机译:非对称旋转航天器的主动章动阻尼:一种Lyapunov设计方法。

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摘要

For small satellites, the attitude architecture of choice is often spin stabilization. Spin stabilization of a satellite about its major axis typically leads to a need for on-board active nutation damping. Spin stabilization of a satellite about its minor axis is typically not considered as a design option, due to the inherent instability of the minor axis spin in the presence of energy dissipation. This work considers the design of nutation damping and spin stabilization systems for small spinning spacecraft.; Nutation damping systems are designed around two distinct actuators. The first actuator considered is a magnetic torque rod, aligned with the desired spin axis, and operated in a bang-bang control mode. The torque rod has the advantage of being simple and inexpensive to build, requiring no expendables, and having extremely high reliability due to its lack of any moving parts. However, magnetic control suffers from the disadvantages of small control torques and limit control authority. The second actuator considered is a small reaction wheel mounted with its axis orthogonal to the desired spin axis. The reaction wheel system also requires no expendables, and is commercially available to satellite designers. Although the reaction wheel is a mechanical system with inherent reliability issues, the technology is mature and has ample spaceflight heritage.; The control law design approach adopted here employs Lyapunov stability theory. Because this technique has not seen extensive use in attitude control applications, we first apply it to attitude stability problems for which the solutions are well understood. Thus, we provide new insight into the stability analysis of the pure spin motions of bodies experiencing energy dissipation. Satisfied that the technique is applicable to the study of spinning bodies, we then employ it to design the active nutation damping control laws of interest. The resulting control laws compare favorably to existing laws found in the literature for each of the actuators considered.
机译:对于小型卫星,选择的姿态架构通常是自旋稳定。卫星绕其主轴的自旋稳定通常导致需要机载主动章动阻尼。卫星绕其短轴的自旋稳定通常不被视为设计选择,因为在存在能量耗散的情况下,短轴自旋的固有不稳定性。这项工作考虑了小型旋转航天器的章动阻尼和自旋稳定系统的设计。振动阻尼系统围绕两个不同的执行器设计。所考虑的第一个执行器是一个磁性扭矩杆,与所需的旋转轴对齐,并在爆炸控制模式下运行。扭矩杆的优点是构造简单且便宜,不需要消耗品,并且由于缺少任何运动部件而具有极高的可靠性。然而,磁控制具有小控制转矩和限制控制权限的缺点。所考虑的第二个致动器是一个小的反作用轮,其轴与所需的旋转轴正交。反作用轮系统也不需要消耗品,卫星设计者可以从市场上买到。尽管反作用轮是具有固有可靠性问题的机械系统,但该技术已经成熟并且具有丰富的航天遗产。这里采用的控制律设计方法采用了Lyapunov稳定性理论。由于该技术尚未在姿态控制应用中得到广泛使用,因此我们首先将其应用于解决方案已经很好理解的姿态稳定性问题。因此,我们为经历能量耗散的物体的纯自旋运动的稳定性分析提供了新的见解。对这项技术适用于纺丝机构的研究感到满意之后,我们将其用于设计感兴趣的主动章动阻尼控制律。对于每个所考虑的执行器,所产生的控制律与文献中发现的现有律相比具有优势。

著录项

  • 作者

    Holden, Timothy Edward.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Engineering Aerospace.
  • 学位 Ph.D.
  • 年度 1999
  • 页码 163 p.
  • 总页数 163
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 航空、航天技术的研究与探索;
  • 关键词

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