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Wavefront sensorless multi-conjugate adaptive optics for imaging in deep atmospheric turbulence: preliminary numerical analysis

机译:用于深层大气湍流成像的波前无传感器多共轭自适应光学器件:初步数值分析

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This paper deals with the problem of imaging in deep atmospheric turbulence conditions such as the ones encountered in long near-horizontal propagation scenarios. Under such conditions, anisoplanatism as well as the presence of intensity scintillations prevent efficient use of conventional single-wavefront corrector adaptive optics systems. Multi-conjugate adaptive optics (MCAO) techniques have been successfully demonstrated in the field of astronomy to mitigate anisoplanatism effects and improve correction on extended objects in weak atmospheric turbulence conditions. However these techniques typically require the use of several wavefront sensors which increases system complexity, and are impacted by the presence of intensity scintillations. We propose to use a wavefront sensorless MCAO method based solely on the optimization of image quality metrics. In this method, the commands applied to the deformable mirrors are computed from a metric derived directly from the compensated image. The method has the advantage of being more robust to scintillations and does not require wavefront sensors. In this preliminary numerical study, we evaluate the benefit of the MCAO approach in deep turbulence.
机译:本文讨论了在深层大气湍流条件下成像的问题,例如在长近水平传播场景中遇到的那些问题。在这种情况下,各向异性和强度闪烁的存在阻碍了传统单波前校正器自适应光学系统的有效利用。多共轭自适应光学(MCAO)技术已在天文学领域得到成功证明,可减轻各向异性影响并改善在弱大气湍流条件下对扩展物体的校正。但是,这些技术通常需要使用几个波前传感器,这会增加系统的复杂性,并且会受到强度闪烁的影响。我们建议仅基于图像质量指标的优化使用波前无传感器MCAO方法。在这种方法中,根据直接从补偿图像得出的度量来计算应用于可变形反射镜的命令。该方法的优点是对闪烁更加鲁棒,并且不需要波前传感器。在此初步的数值研究中,我们评估了MCAO方法在深湍流中的优势。

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