近地轨道
光圈(计算机存储器)
地铁列车时刻表
光学
遥感
物理
合成孔径雷达
航空航天工程
轨道(动力学)
计算机科学
天文
卫星
工程类
地质学
人工智能
声学
操作系统
作者
S. Chakrabarti,Gerard L. Rafanelli,Susan Spencer,Douglas W. Wolfe,R. S. Polidan,Christopher M. Cosner,Arthur M. Newman
摘要
We describe a paradigm shift for astronomical observatories that would replace circular apertures with rotating synthetic apertures. Rotating Synthetic Aperture (RSA) observatories can enable high value science measurements for the lowest mass to orbit, have superior performance relative to all sparse apertures, can provide resolution of 20m to 30m apertures having the collecting area of 8m to 12m telescopes with much less mass, risk, schedule, and cost. RSA is based on current, or near term technology and can be launched on a single, current launch vehicle to L2. Much larger apertures are possible using the NASA Space Launch System.
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