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Acceleration of AO simulation using programmable logic

机译:使用可编程逻辑加速AO仿真

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摘要

Numerical Simulation is an essential part of the design and optimisation of astronomical adaptive optics systems. Simulations of adaptive optics are computationally expensive and the problem scales rapidly with telescope aperture size, as the required spatial order of the correcting system increases. Practical realistic simulations of AO systems for extremely large telescopes are beyond the capabilities of all but the largest of modern parallel supercomputers. Here we describe a more cost effective approach through the use of hardware acceleration using field programmable gate arrays. By transferring key parts of the simulation into programmable logic, large increases in computational bandwidth can be expected. We show that the calculation of wavefront sensor images (involving a 2D FFT, photon shot noise addition, background and readout noise), and centroid calculation can be accelerated by factor of 400 times when the algorithms are transferred into hardware. We also provide details about the simulation platform and framework that we have developed at Durham.
机译:数值模拟是天文自适应光学系统设计和优化的重要组成部分。自适应光学系统的仿真计算量很大,并且随着校正系统所需空间顺序的增加,该问题随望远镜孔径的大小迅速扩大。除了最大型的现代并行超级计算机之外,用于超大型望远镜的AO系统的实际仿真都超出了所有其他模型的能力。在这里,我们通过使用现场可编程门阵列的硬件加速来描述一种更具成本效益的方法。通过将仿真的关键部分转换为可编程逻辑,可以预期计算带宽的大幅增加。我们表明,将算法转移到硬件中后,波前传感器图像(涉及2D FFT,光子散粒噪声,背景和读出噪声)的计算和质心计算可以加速400倍。我们还将提供有关我们在达勒姆(Durham)开发的仿真平台和框架的详细信息。

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