多共轭自适应光学系统倾斜各向异性的斜率合并方法

Hao Zhang, Jesse Cranney, D. Gratadour, N. Doucet, F. Rigaut
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引用次数: 0

摘要

大型光学望远镜依靠自适应光学来实时补偿湍流引起的波前像差。基于激光导星的多共轭自适应光学系统的倾斜各向异性影响了系统的性能。在本文中,我们提出并推导了一种减轻这种影响的方法,该方法通过将自然星和激光导星的测量合并在一起来实现。该方法对高阶激光导星无法感知的场相关倾斜像差进行模态重建。该方法的优点是:(i)减少了计算量,(ii)与预测控制方案兼容,(iii)提高了整个科学视场图像质量的均匀性。通过端到端数值模拟验证了斜率合并方法在现代自适应光学系统中的性能。
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Mitigating Tilt Anisoplanatism with the Slope Merging Method for Multi-Conjugate Adaptive Optics Systems
Large optical telescopes depend on adaptive optics for the real-time compensation of turbulence-induced wavefront aberrations. The performance of laser guide star based Multi-Conjugate Adaptive Optics systems is degraded by tilt anisoplanatism. In this paper we propose and derive a method for mitigating this effect, achieved by merging the measurements of natural and laser guide stars together. This method performs a modal reconstruction of the field dependent Tip-Tilt aberration that is not sensed by the high order laser guide stars. The proposed method benefits from its (i) reduced computational load, (ii) compatibility with predictive control schemes, and (iii) improved uniformity of image quality over the whole science field of view. End-to-end numerical simulations are used to demonstrate the performance of the slope merging method in modern Adaptive Optics systems.
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