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Telescope performance near local midnight for the Japanese Advanced Meteorological Imager (JAMI)

机译:日本先进气象成像仪(JAMI)在当地午夜附近的望远镜性能

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Raytheon's Santa Barbara Remote Sensing (SBRS) division designed and built the MTSAT-1R Japanese Advanced Meteorological Imager for the Japanese Ministry of Transport between March, 1999 and July, 2002. In order to meet the stressing requirements of a geosynchronous orbit, a combination of structural, thermal, and optical (STOP) analyses were used to design and optimize the beryllium three-mirror anastigmat (TMA) telescope. This modeling approach was used to characterize and minimize the thermal distortion around local midnight. On-orbit temperatures and structural deformations were predicted using thermal Desktop/SINDA and PATRAN/NASTRAN software, respectively. The resulting optical performance was evaluated using Raytheon developed HEXAGON software. The telescope design was successfully optimized to attain specified visible channel performance for most of the 24 hour orbit.
机译:雷神公司的圣塔芭芭拉遥感(SBRS)部门在1999年3月至2002年7月之间为日本交通运输部设计并建造了MTSAT-1R日本先进气象成像仪。为了满足地球同步轨道的压力要求,使用结构,热和光学(STOP)分析来设计和优化铍三反射镜(TMA)望远镜。该建模方法用于表征和最小化局部午夜附近的热变形。使用热Desktop / SINDA和PATRAN / NASTRAN软件分别预测在轨温度和结构变形。使用Raytheon开发的HEXAGON软件评估所得的光学性能。望远镜设计已成功优化,以在24小时轨道的大部分时间内达到指定的可见通道性能。

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