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International Space Station rate gyro alignment estimation

机译:国际空间站速率陀螺仪对准估计

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摘要

Two Rate Gyro Assemblies (RGAs) are used by the International Space Station (ISS) onboard Navigation function as a source of vehicle attitude rates. Prior to flight, it was necessary to make physical measurements of the actual achieved mounting orientation of these RGAs, relative to a fiducial reference frame embedded in the ISS truss structure. The resulting measurements were used to calculate initialization data for the flight software, and also provided a basis for a statistical statement relative to correct installation of the RGAs. The measurement process was accomplished using LASER ranging and angles data to establish inertial positions of several locations on the RGA optical cubes. A Least Squares Differential Correction (LSDC) process was used to yield an optimal estimate of the orientation of each RGA. Since the measurements set was not large, confidence intervals were used for statistical interpretation of the results.
机译:国际空间站(ISS)的机载导航功能使用两个速率陀螺仪组件(RGA)作为车辆姿态速率的来源。飞行之前,有必要相对于ISS桁架结构中嵌入的基准参考框架对这些RGA的实际实现的安装方向进行物理测量。所得的测量结果用于计算飞行软件的初始化数据,并且还为有关RGA正确安装的统计声明提供了基础。使用LASER测距和角度数据在RGA光学立方体上建立几个位置的惯性位置,即可完成测量过程。最小二乘差分校正(LSDC)过程用于产生每个RGA方向的最佳估计。由于测量值集不大,因此将置信区间用于结果的统计解释。

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