使用连接机的自适应光学计算

R. Firestone, Eric N. Opp
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引用次数: 0

摘要

位于地球表面的反射式光学望远镜,由于反射镜上的重力作用和光路上大气的湍流,其性能会受到畸变。反射光学也计划用于高功率激光系统,其中光本身的强度能够在仪器内的空气中产生扭曲,从而影响聚焦波前的形状。光学设计师提出的一种解决方案是使用自适应光学:一种光学系统,其中镜子的形状可以变形到必要的程度,以纠正所提到的畸变。自适应光学系统使用反馈回路概念,测量光波前的畸变,计算必要的校正,并移动一组致动器来提供这些校正。修正的计算需要大量的计算。具体来说,对畸变的测量提供了与致动器位置对应的测量点之间相位差的集合。这组相位差大于执行器的数量,导致过定问题。由于物理系统存在一定数量的噪声,最小二乘解决技术既可以为这种超定问题提供执行器位置的最佳选择,又可以抑制测量中的噪声。解决自适应光学问题计算部分的必要算法包括导出物理系统计算表示的矩阵生成器、矩阵反演程序和高速最小二乘求解器。在光学天文学范式中,由于大气湍流的速率,计算要求是每秒进行少量调整。对于要求更严格的激光系统,我们展示了11.2个数量级的改进,只有通过使用超级计算机方法才能实现。这些结果的外推表明,如果处理器间通信最小化,甚至可能有更大的加速;换句话说,超级计算机设计者还没有解决如何使处理器间的通信像处理器内部的通信那样高效的问题(或者,在目前的情况下,在单个芯片上的处理器之间的通信)。
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Adaptive Optics Calculations Using the Connection Machine
The performance of reflecting optical telescopes located on the surface of the earth are subject to distortions due to the force of gravity on the mirror and the turbulence of the atmosphere on the light path. Reflective optics are also planned for use in high-powered laser systems, where the intensity of the light itself is capable of producing distortions in the air within the instrument, thereby affecting the shape of the focused wavefront. A solution proposed by optical designers is the use of adaptive optics: an optical system in which the figure of the mirror is deformable to the extent necessary to correct for the distortions mentioned. An adaptive optical system uses a feedback loop concept, in which the distortions of the optical wavefront are measured, the necessary corrections are computed, and a set of actuators is moved to provide those corrections. The calculation of the corrections is computationally intense. Specifically, the measurement of the distortions provides a collection of phase differences between measuring points corresponding to the actuator positions. This set of phase differences is larger than the number of actuators, leading to an overdetermined problem. As physical systems have some amount of noise present, the technique of least-squares solution serves both to provide the best choice of actuator positions for this overdetermined problem and to suppress the noise in the measurements. The necessary algorithms for solving the computation portion of the adaptive optics problem consist of a matrix generator to derive the computational representation of the physical system, a matrix inversion routine, and a high-speed least-squares solver. In the optical astronomy paradigm, the computational requirement is for a small number of adjustments per second, due to the rate of atmospheric turbulence. For the laser system, with more stringent requirements, we demonstrate an improvement of 11 2 orders of magnitude, made possible only through the use of supercomputer methods. Extrapolation of these results indicates that even greater acceleration is possible if the interprocessor communication is minimized; in other words, supercomputer designers have not yet solved the problem of making interprocessor communication as efficient as that within processors (or, in the present case, between processors on a single chip).
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