首页> 外文期刊>Journal of the Optical Society of America, A. Optics, image science, and vision >On the optimal reconstruction and control of adaptive optical systems with mirror dynamics
【24h】

On the optimal reconstruction and control of adaptive optical systems with mirror dynamics

机译:具有镜面动力学的自适应光学系统的最优重构和控制

获取原文
获取原文并翻译 | 示例
获取外文期刊封面目录资料

摘要

In adaptive optics (AO) the deformable mirror (DM) dynamics are usually neglected because, in general, the DM can be considered infinitely fast. Such assumption may no longer apply for the upcoming Extremely Large Telescopes (ELTs) with DM that are several meters in diameter with slow and/or resonant responses. For such systems an important challenge is to design an optimal regulator minimizing the variance of the residual phase. In this contribution, the general optimal minimum-variance (MV) solution to the full dynamical reconstruction and control problem of AO systems (AOSs) is established. It can be looked upon as the parent solution from which simpler (used hitherto) suboptimal solutions can be derived as special cases. These include either partial DM-dynamics-free solutions or solutions derived from the static minimum-variance reconstruction (where both atmospheric disturbance and DM dynamics are neglected altogether). Based on a continuous stochastic model of the disturbance, a state-space approach is developed that yields a fully optimal MV solution in the form of a discrete-time linear-quadratic-Gaussian (LQG) regulator design. From this LQG standpoint, the control-oriented state-space model allows one to (1) derive the optimal state-feedback linear regulator and (2) evaluate the performance of both the optimal and the sub-optimal solutions. Performance results are given for weakly damped second-order oscillatory DMs with large-amplitude resonant responses, in conditions representative of an ELT AO system. The highly energetic optical disturbance caused on the tip/tilt (TT) modes by the wind buffeting is considered. Results show that resonant responses are correctly handled with the MV regulator developed here. The use of sub-optimal regulators results in prohibitive performance losses in terms of residual variance; in addition, the closed-loop system may become unstable for resonant frequencies in the range of interest.
机译:在自适应光学(AO)中,通常忽略可变形镜(DM)的动力学,因为通常可以将DM无限快地考虑在内。这种假设可能不再适用于即将推出的直径为几米,速度较慢和/或共振的DM的超大型望远镜(ELT)。对于这样的系统,一个重要的挑战是设计一种最小化残余相位变化的最佳调节器。在此贡献中,建立了针对AO系统(AOS)的完整动态重构和控制问题的一般最优最小方差(MV)解决方案。可以将其视为父解决方案,从中可以得出更简单的(迄今为止使用的)次优解决方案作为特殊情况。这些包括无局部DM动力学解或源自静态最小方差重构的解决方案(其中完全忽略了大气干扰和DM动力学)。基于干扰的连续随机模型,开发了一种状态空间方法,该方法以离散时间线性二次高斯(LQG)调节器设计的形式产生了完全最佳的MV解决方案。从这种LQG的角度来看,面向控制的状态空间模型允许(1)推导最佳状态反馈线性调节器,以及(2)评估最佳和次优解决方案的性能。在代表ELT AO系统的条件下,给出了具有大幅度共振响应的弱阻尼二阶振荡DM的性能结果。考虑了由风抖动在尖端/倾斜(TT)模式上引起的高能光学干扰。结果表明,使用此处开发的MV调节器可以正确处理谐振响应。使用次优的调节器会导致残余方差方面的性能损失;另外,对于所关注范围内的谐振频率,闭环系统可能变得不稳定。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号