Nonlinear plate equation analysis for the design of large stroke deformable mirror

SPIE MOEMS-MEMS Pub Date : 2008-02-27 DOI:10.1117/12.766873
Oscar A. Azucena, B. Fernández, J. Kubby
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引用次数: 4

Abstract

Adaptive Optics (AO) improves the quality of astronomical imaging systems by using real time measurement of the turbulent medium in the optical path. The measurements are then taken and applied to a deformable mirror (DM) that is in the conjugate position of the aberrations in the optical path. The quality of the reconstructed wavefront directly affects the images obtained. One of the limiting factors in current DM technology is the amount of stroke available to correct the wavefront distortions which can be as high as 20 microns of optical path difference. We have developed a simulation analysis using Galerkin's method to solve the nonlinear plate equation. The analysis uses a set of orthogonal equations that satisfied the boundary condition to solve for the linear deformation on the mirror surface. This deformation is used to iteratively converge to the final solution by applying the nonlinear plate equation and the nonlinear actuator forces. This simulation was used to design a microelectromechanical DM with 10 μm of stroke.
大行程变形镜设计的非线性板方程分析
自适应光学(AO)通过对光路湍流介质的实时测量来提高天文成像系统的质量。然后测量并应用于光路中像差共轭位置的可变形镜(DM)。重建波前的质量直接影响得到的图像。当前DM技术的限制因素之一是可用于校正波前畸变的冲程量,这种波前畸变可高达20微米的光程差。本文采用伽辽金法对非线性板方程进行了模拟分析。利用一组满足边界条件的正交方程求解镜面的线性变形。利用这种变形,利用非线性板方程和非线性作动器力迭代收敛到最终解。利用该仿真设计了行程为10 μm的微机电DM。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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