Optimization of the Starfire Optical Range 3.5 M adaptive optics for astronomical imaging

D. Link, R. Vernon
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Abstract

SAIC has developed a wave-optics, time domain, engineering simulation of adaptive optics systems. The Atmospheric Compensation Simulation (ACS) includes both physics effects (e.g., inner and outer scale, various turbulence profiles, wind, anisoplanatism, time of flight, scattering, absorption, sodium layer saturation) and engineering effects (e.g. jitter, misregistration, latency, digital controls, control surface electro-mechanical response, gain variation, shot and detector noise, quantization, aberrations). The code includes the ability to model multiple three-dimensional laser guidestars, propagating the lasers up from the ground and imaging the irradiance from multiple atmospheric layers onto the detector plane using multiple optical transfer functions or speckle imaging. This simulation has been used to support engineering development on a number of programs and has been validated against theory, experiments, and other codes.
Starfire光学距离3.5 M天文成像自适应光学系统的优化
SAIC开发了波光学、时域、工程仿真的自适应光学系统。大气补偿模拟(ACS)包括物理效应(如内外尺度、各种湍流剖面、风、各向异性、飞行时间、散射、吸收、钠层饱和度)和工程效应(如抖动、错配、延迟、数字控制、控制面机电响应、增益变化、射击和探测器噪声、量化、像差)。该代码包括模拟多个三维激光导星的能力,从地面传播激光,并利用多个光学传递函数或散斑成像将多个大气层的辐照度成像到探测器平面上。该模拟已用于支持许多程序的工程开发,并已根据理论、实验和其他代码进行了验证。
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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