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Fault Detection and Correction for the Solar Dynamics Observatory Attitude Control System

机译:太阳动力天文台姿态控制系统的故障检测与纠正

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The Solar Dynamics Observatory is an Explorer-class mission that will launch in December, 2008. The spacecraft will operate in a geosynchronous orbit, sending data 24 hours a day to a devoted ground station in White Sands, New Mexico. It will carry a suite of instruments designed to observe the Sun in multiple wavelengths at unprecedented resolution. The Atmospheric Imaging Assembly includes four telescopes with focal plane CCDs that can image the Ml solar disk in four different visible wavelengths. The Extreme-ultraviolet Variability Experiment will collect time-correlated data on the activity of the Sun's corona. The Helioseismic and Magnetic Imager will enable study of pressure waves moving through the body of the Sun. The attitude control system on Solar Dynamics Observatory is responsible for four main phases of activity. The physical safety of the spacecraft after separation must be guaranteed. Fine attitude determination and control must be sufficient for instrument calibration maneuvers. The mission science mode requires 2-arcsecond control according to error signals provided by guide telescopes on the Atmospheric Imaging Assembly, one of the three instruments to be carried. Lastly, accurate execution of linear and angular momentum changes to the spacecraft must be provided for momentum management and orbit maintenance. In this paper, single-fault tolerant fault detection and correction of the Solar Dynamics Observatory attitude control system is described. The attitude control hardware suite for the mission is catalogued, with special attention to redundancy at the hardware level. Four reaction wheels are used where any three are satisfactory. Four pairs of redundant thrusters are employed for orbit change maneuvers and momentum management. Three two-axis gyroscopes provide full redundancy for rate sensing. A digital Sun sensor and two autonomous star trackers provide two-out-of-three redundancy for fine attitude determination. The use of software to maximize chances of recovery from any hardware or software fault is detailed. A generic fault detection and correction software structure is used, allowing additions, deletions, and adjustments to fault detection and correction rules. This software structure is fed by in-line fault tests that are also able to take appropriate actions to avoid corruption of the data stream.
机译:太阳动力天文台是探险家级的任务,将于2008年12月发射。该航天器将在地球同步轨道上运行,每天24小时将数据发送到新墨西哥州白沙的一个专用地面站。它将携带一套旨在以前所未有的分辨率观察多个波长的太阳的仪器。大气成像组件包括具有焦平面CCD的四个望远镜,其可以在四个不同的可见波长下对M1太阳盘成像。极端紫外线变异性实验将收集与太阳日冕活动相关的时间相关数据。 Helioseismic和Magnetic成像仪将使研究穿过太阳身体的压力波成为可能。太阳动力天文台的姿态控制系统负责活动的四个主要阶段。分离后必须保证航天器的人身安全。良好的姿态确定和控制必须足以进行仪器校准。任务科学模式需要根据大气成像组件上的导向望远镜提供的误差信号进行2秒控制,这是要携带的三种仪器之一。最后,必须提供对航天器线性和角动量变化的准确执行,以进行动量管理和轨道维护。本文描述了太阳动力天文台姿态控制系统的单容错故障检测和纠正。对用于任务的姿态控制硬件套件进行了分类,并特别注意了硬件级别的冗余性。当三个反作用轮令人满意时,使用四个反作用轮。四对冗余推力器用于改变轨道的动量和动量管理。三个三轴陀螺仪为速率感测提供了完全的冗余。一个数字阳光传感器和两个自主恒星跟踪器可提供三分之二的冗余度,以进行精细的姿态确定。详细介绍了如何使用软件来最大化从任何硬件或软件故障中恢复的机会。使用通用的故障检测和纠正软件结构,允许添加,删除和调整故障检测和纠正规则。该软件结构由在线故障测试提供支持,这些故障测试也能够采取适当的措施以避免数据流损坏。

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