【24h】

Simulations of high order curvature adaptive optics

机译:高阶曲率自适应光学仿真

获取原文

摘要

CFHT recently considered an upgrade of its curvature adaptive optics system to perform high dynamic range imaging. This requires high Strehl ratios and very stable Point Spread Functions, which is usually achieved with high order AO systems providing a dense sampling and correction across the pupil. Such systems are conventionally thought of as Shack-Hartman/piezostack devices because, in theory the scaling law for noise propagation goes as N.log(N), where N is the number of actuators. However, it is difficult to demonstrate this behavior in practice, and as systems get more complex, their efficiency drops to lower levels than expected. Simulations of such systems are usually optimistic because the fail to take the complexity of a real system's flaws (alignment errors, imperfect lenslet array, etc.) into account. One of the reasons why curvature adaptive optics looses its efficiency advantage for large numbers of degrees of freedom is because of its noise propagation properties. The exact crossover with Shack-Hartman systems in terms of performance and efficiency remains to be determined, but cheap (and may be more reliable) high dynamic range systems on smaller telescopes could conceivably use curvature technology. When the number of degrees of freedom remains low, realistic Monte Carlo simulations are possible and provide a more accurate benchmark, as the computing time remains reasonnable. Monte Carlo simulations of such a system have been performed in view of upgrading PUEO, the CFHT adaptive optics bonnette, as a test bench for high dynamic range imaging, and for visible adaptive optics (Lai et al, these proceedings [4839-78]). Simulations show that 104 subapertures/electrode are sufficient to produce a Strehl ratio of 92in K band (S(I) = 5821 However, because PSF stability is so critical and the noise propagation is crucial to the performance, we are hoping to test this system on different simulation codes to confirm these results and expand on them using specificity of each code to complement the other. As this is work in progress, this paper will concentrate on the road ahead and the advantages and drawbacks of each code for each specific task.
机译:CFHT最近考虑了升级其曲率自适应光学系统,以执行高动态范围成像。这需要高刻度比和非常稳定的点传播功能,这通常通过高阶AO系统实现,提供致密的采样和穿过瞳孔的校正。这些系统通常被认为是Shack-Hartman / PieZostack装置,因为理论上,用于噪声传播的缩放法作为N.log(n),其中n是执行器的数量。然而,很难在实践中展示这种行为,并且随着系统变得更加复杂,它们的效率降低了比预期的更低。这种系统的模拟通常是乐观的,因为无法考虑真实系统的缺陷(对准错误,不完全定位镜头等)的复杂性。曲率自适应光学器件损失其大量自由度的效率优势的原因之一是因为其噪声传播特性。在性能和效率方面,与Shack-Hartman系统的确切交叉仍有待确定,但较低望远镜上的高动态范围系统可以想到使用曲率技术。当自由度的程度仍然很低时,现实的蒙特卡罗模拟是可能的并且提供更准确的基准,因为计算时间仍然是合理的。在升级Pueo,CFHT自适应光学博内特的升级Pueo,作为高动态范围成像的测试台,以及可见自适应光学器件(Lai等,这些诉讼[4839-78]),已经执行了这种系统的蒙特卡罗模拟。[4839-78] 。仿真表明,104个子镜/电极足以产生92in k带的刻度比(S(i)= 5821,因为PSF稳定性是如此关键,并且噪声传播对性能至关重要,我们希望测试该系统在不同的仿真代码上,以确认这些结果并使用每个代码的特殊性来扩展它们以补充另一个。由于这是在进行中的工作,本文将专注于前方的道路以及每个特定任务的每个代码的优势和缺点。

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