On Orbit Performance of the Hubble Space Telescope Fine Guidance System Operating in the Coarse Track Mode

R. Whittlesey
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Abstract

The Hubble Space Telescope (HST) Fine Guidance System (FGS) was designed and demonstrated to provide a robust Coarse Track capability with a pointing accuracy of .02 arc second rms when tracking a Mv 14.5 star. Orbital data indicates that tracking performance varies from .02 to .065 arc second (Bely and Liu). Two HST hardware characteristics are identified as contributing to the higher than expected pointing errors. High jitter levels are induced by Solar Array Assembly mechanical shocks during and following day/night orbital transitions. Reduced signal to noise performance occurs in the Coarse Track control loop because of the spherically aberrated images from the telescope optics. A Computer simulation has been developed to investigate the operation of the Coarse Track mode performance and to determine if performance can be enhanced by modification of up-link control variables.
粗轨模式下哈勃空间望远镜精细制导系统的轨道性能研究
哈勃太空望远镜(HST)精细制导系统(FGS)的设计和演示提供了强大的粗跟踪能力,在跟踪Mv 14.5的恒星时,指向精度为0.02角秒。轨道数据表明,跟踪性能在0.02到0.065角秒之间变化(Bely和Liu)。两个HST硬件特性被认为是导致指向误差高于预期的原因。高抖动水平是由太阳能电池阵列组件在昼夜轨道转换期间和之后的机械冲击引起的。由于望远镜光学系统的球像差,导致粗轨道控制回路的信噪比降低。计算机仿真研究了粗航迹模式性能的运行,并确定是否可以通过修改上行链路控制变量来提高性能。
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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