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An in-flight alignment calibration scheme for astronomy telescope

机译:天文望远镜的飞行校准校准方案

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Developing the observation technology in space astronomy science, to realize accurate pointing control and/or to determine accurate direction of the observing objects are strongly required. However, it is difficult to be free from the problem of the distortion of the satellite structure or the telescope itself that is induced by thermally or other complex phenomena. These distortion cause analysis error in the observation analysis. This paper proposes a solution. In this scheme, several displacement-measuring equipments are introduced and the outputs of this monitor system are sending to ground-station. This scheme is assuming the linearity of the relation between the distortion and observed results by mission instrument (such as space telescope). Once this basic assumption is accepted, it becomes to be able to use mathematical linear theory for alignment analysis. As the results, it enables to compensate observing data to perform the calibration operation in orbit.
机译:在太空天文学中开发观察技术,实现准确的指导控制和/或确定观察物体的准确方向。然而,难以摆脱卫星结构的变形或望远镜本身的问题,该望远镜本身是通过热或其他复杂现象诱导的。这些失真导致观察分析中的分析误差。本文提出了解决方案。在该方案中,引入了几种位移测量设备,并且该监视系统的输出正在发送到地站。该方案假设由任务仪器(例如太空望远镜)的失真与观察结果之间的关系的线性。一旦接受了这种基本假设,就能使用数学线性理论进行对准分析。结果,它使得能够补偿观察数据以在轨道中执行校准操作。

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