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Modified deformable mirror stroke minimization control for direct imaging of exoplanets

机译:改进的可变形镜面行程最小化控制,可对系外行星进行直接成像

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For direct imaging of faint exoplanets, coronagraphs are widely used to suppress light and achieve a high contrast. Wavefront correction algorithms based on adaptive optics are introduced simultaneously to mitigate aberrations in the optical system. Stroke minimization is one of the primary control algorithms used for high-contrast wavefront control. This technique calculates the minimum deformation across the deformable mirrors' surface under the constraint that a targeted average contrast level in the search areas, namely the dark holes, is achieved. In this paper we present a modified linear constraint stroke minimization algorithm. Instead of using a single constraint on intensity averaged over all pixels, we constrain the electric field's real and imaginary part of each pixel in the dark holes. The new control algorithm can be written into a linear programming problem. Model reduction methods, including pixel binning and singular value decomposition (SVD), are further employed to avoid over-constraining the problem and to speed up computation. In numerical simulation, we find that the revised algorithm leads to more uniform dark holes and faster convergence.
机译:为了对微弱的系外行星进行直接成像,日冕仪被广泛用于抑制光线并获得高对比度。同时引入了基于自适应光学的波前校正算法,以减轻光学系统中的像差。冲程最小化是用于高对比度波前控制的主要控制算法之一。该技术在可实现搜索区域(即黑洞)目标平均对比度水平的约束下,计算出可变形反射镜表面的最小变形。在本文中,我们提出了一种改进的线性约束笔划最小化算法。我们没有对所有像素的平均强度使用单一约束,而是限制了黑洞中每个像素的电场的实部和虚部。新的控制算法可以写入线性规划问题。还采用了模型缩减方法,包括像素合并和奇异值分解(SVD),以避免过度约束问题并加快计算速度。在数值模拟中,我们发现改进的算法导致更均匀的黑洞和更快的收敛。

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