最优波前估计和控制采用自适应技术

Tyler Groff, N. Kasdin
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引用次数: 3

摘要

用于类地行星探测的天基日冕仪将需要焦平面波前控制以达到必要的对比度水平。这些校正算法是迭代的,需要对科学摄像机的电场进行估计。为了使科学时间最大化,必须尽量减少校正时间,这意味着减少校正所需的曝光次数。这也意味着最小化迭代次数和每次迭代的曝光次数,以达到目标对比度。理想的选择是使用较少的曝光来估计电场,并具有相同的精度水平。我们展示了一个最优估计器,它使用先验知识来创建电场的估计。将该方法的性能与旨在给出最小二乘最小误差的两两估计器进行了比较。这使我们能够评估达到对比度目标所需的图像数量。
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Optimal wavefront estimation and control using adaptive techniques
Space-based coronagraphs for earth-like planet detection will require focal plane wavefront control to achieve the necessary contrast levels. These correction algorithms are iterative and require an estimate of the electric field at the science camera. In order to maximize science time the correction time must be minimized, which means reducing the number of exposures required for correction. This also means minimizing the number of iterations and the number of exposures per iteration to achieve a targeted contrast. The ideal choice is to use fewer exposures to estimate the electric field with the same level of accuracy. We demonstrate an optimal estimator that uses prior knowledge to create the estimate of the electric field. The performance of this method is compared to a pairwise estimator which is designed to give the least-squares minimal error. This allows us to evaluate the number of images necessary to achieve a contrast target.
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