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Using 50-mm electrostatic membrane deformable mirror in astronomical adaptive optics

机译:在天文自适应光学中使用50毫米静电膜可变形镜

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Membrane micro-machined deformable mirrors (MMDM) feature low cost, low power consumption, small size and absence of hysteresis. Interested in using such a device for the adaptive optics system at the SOAR 4.1-m telescope, we evaluated the performance of a 79-channel 50-mm (pupil size 35mm) MMDM from OKO Technologies. The measured influence functions match the solutions of the Poisson equation with a fixed boundary. The maximum achievable modulation of the local radius of curvature of the mirror is +-25 m. Simulations of the AO system with this MMDM show that the curvature saturation becomes apparent even at a median seeing of 0.67″. A new control algorithm that re-distributes the signals of saturated electrodes to adjacent ones significantly improves compensation under conditions of partial saturation. Limited curvature range and pupil diameter restrict the suitability of MMDM technology to moderate order AO systems at telescopes with diameter of up to 3m.
机译:膜微机械可变形镜(MMDM)具有成本低,功耗低,尺寸小和没有滞后的特点。有兴趣在SOAR 4.1-m望远镜上将这种设备用于自适应光学系统,我们评估了OKO Technologies的79通道50mm(瞳孔尺寸35mm)MMDM的性能。测得的影响函数与具有固定边界的泊松方程的解匹配。镜子局部曲率半径的最大可实现调制为+ -25 m。使用该MMDM的AO系统的仿真表明,即使在看到0.67英寸的中间值时,曲率饱和也会变得明显。一种将饱和电极信号重新分配给相邻电极的新控制算法,可以显着改善部分饱和条件下的补偿。有限的曲率范围和瞳孔直径将MMDM技术的适用性限制在直径最大3m的望远镜上适合中等阶数的AO系统。

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