Precision space telescope attitude determination and control system design principles

A. V. Fateev, Y. V. Vilkov, V. E. Chebotarev, M. G. Matylenko, G. P. Titov
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Abstract

In order to preclude the impact of atmospheric factors on the quality of received data, state of the art astronomy research projects require spacecraft mounted telescopes. However, such designs entail the issue of sustaining the accuracy of telescope boresight attitude relative to the object of observation for the required period of time. This paper is a summary of design principles for an attitude determination and control system of a space telescope mounted rigidly onboard a spacecraft. The paper formulates requirements for attitude accuracy, and proposes a viable equipment configuration as well as a three- stage attitude control algorithm. The first stage of the algorithm ensures primary boresight pointing towards the target object prior to the object being captured in the telescope’s FoV based on star tracker and angular rate sensor data. The second stage of the algorithm ensures boresight positioning relative to the target object direction up to an error value allowing for the required image quality, based on telescope readings. The third stage of the algorithm ensures telescope boresight holding relative to the target object direction with a required accuracy for the duration of exposure. Interferences from operating satellite equipment are reviewed, and the principles of reducing their impact on sighting accuracy are formulated. Low inclination, low eccentricity geostationary orbit is recommended as the best operating environment for the space telescope’s scientific instrumentation, as well as for providing a continuous data interface between spacecraft and ground segment.
精密空间望远镜姿态确定和控制系统设计原理
为了排除大气因素对接收数据质量的影响,最先进的天文学研究项目需要安装航天器望远镜。然而,这种设计需要在所需的时间内保持望远镜相对于观测对象的内窥姿态的准确性。本文概述了刚性安装在航天器上的空间望远镜的姿态确定和控制系统的设计原则。论文提出了对姿态精度的要求,并提出了可行的设备配置和三阶段姿态控制算法。该算法的第一阶段是根据星轨和角速率传感器数据,确保在望远镜视场捕捉到目标物体之前,将主内径指向目标物体。算法的第二阶段是根据望远镜读数,确保相对于目标物体方向的孔径定位,误差值不超过所需的图像质量。算法的第三阶段确保在曝光持续时间内,望远镜孔径相对于目标物体方向的保持达到所要求的精度。对运行中的卫星设备的干扰进行了审查,并制定了减少其对瞄准精度影响的原则。建议将低倾角、低偏心率地球静止轨道作为空间望远镜科学仪器的最佳操作环境,并为航天器和地面部分提供连续的数据接口。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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