美国宇航局深空网络
波前
光学
望远镜
自由空间光通信
自适应光学
光束发散
激光器
物理
火星探测计划
光圈(计算机存储器)
斯皮策太空望远镜
遥感
激光束质量
计算机科学
航天器
激光束
地质学
天文
声学
作者
David Driscoll,Brian Zellers,Jason Schomacker,John Carro,D. MacDonald,W. T. Roberts,James Guregian,William Klipstein
摘要
Maintaining a stable and high quality laser wavefront is pivotal for efficient laser communications in deep space networks. In this presentation, we describe the design and expected optical and structural performance of the afocal beam expanding telescope for the NASA DSOC mission. This 22 cm aperture, 11x magnification telescope must survive the stresses of launch and maintain alignment through solar illumination, laser irradiance, thermal transients, and temperature extremes during the DSOC mission life from Earth to Mars. Structural-Thermal-OPtical (STOP) analysis predict very stable downlink wavefront error (< 122 nm RMS) and beam divergence (< 14.5 microradians). Furthermore, we present additional telescope link loss contributions that will be minimized through particulate contamination control, high spectral throughput, and polarization purity. Successful performance of this telescope will support NASA's ongoing efforts to extended high data rate communications into deep space.
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