地球静止轨道自旋卫星姿态确定及控制策略

本文从工程应用的角度详尽地介绍了地球静止轨道自旋卫星姿态原理及确定方法,以我国在轨运行的风云二号卫星为例,给出了大量工程实测数据,并给出姿态控制实施策略,它们已经成功地运用到我国在轨自旋同步卫星的管理。     

两轴稳定平台的过顶盲区问题

过顶盲区问题是目标在导弹的小离轴角附近区域运动时,由于框架角速率限制产生的稳定平台不能正常跟踪目标机动的一种现象.根据光电探测系统成像的几何关系,分别对直角坐标框架和极坐标框架稳定平台的目标成像关系进行了分析,进而给出极坐标框架稳定平台的过顶盲区的数学描述,并对这种盲区的成因进行了分析.结合三种情况的目标机动速度,在Matlab的Simulink环境下对极坐标框架稳定平台的过顶盲区现象进行了仿真.最后,基于分区域变参数的PID控制方法,给出了目标在过顶盲区内作垂直向上机动时的一种控制方案,并与普通PID控制进行了对比仿真研究.实际仿真结果表明,通过数学分析得到的极坐标框架稳定平台的过顶盲区模型与实际情况相符合,并且基于分区域变参数的PID控制方法能够改善极坐标框架稳定平台的跟踪特性.      

基于TMS320F2812的卫星天线稳定控制系统的设计

对卫星天线稳定跟踪系统的工作原理进行了分析,设计了一种基于DSP TMS320F2812的天线稳定控制器,详细分析了系统的原理、构成、设计方法,概要介绍了DSP芯片的特点及其电路设计和系统软件的设计及其模块划分和功能,在matlab上对系统进行了仿真实验,得到了良好的仿真效果。     

CXG—2型磁悬规转子横向稳定的研究

本文针对CXG-1型磁悬规的转子横向振动现象进行了分析探讨,提出CXG-2型磁悬规的转子横向阻尼方案,并给出实施后的实验结果。     

Spin motion determination of the Envisat satellite through laser ranging measurements from a single pass measured by a single station

The Satellite Laser Ranging (SLR) technology is used to accurately determine the position of space objects equipped with so-called retro-reflectors or retro-reflector arrays (RRA). This type of measurement allows to measure the range to the spacecraft with high precision, which leads to determination of very accurate orbits for these targets. Non-active spacecraft, which are not attitude controlled any longer, tend to start to spin or tumble under influence of the external and internal torques and forces.If the return signal is measured for a non-spherical non-active rotating object, the signal in the range residuals with respect to the reference orbit is more complex. For rotating objects the return signal shows an oscillating pattern or patterns caused by the RRA moving around the satellite’s centre of mass. This behaviour is projected onto the radial component measured by the SLR.In our work, we demonstrate how the SLR ranging technique from one sensor to a satellite equipped with a RRA can be used to precisely determine its spin motion during one passage. Multiple SLR measurements of one target over time allow to accurately monitor spin motion changes which can be further used for attitude predictions. We show our solutions of the spin motion determined for the non-active ESA satellite Envisat obtained from measurements acquired during years 2013–2015 by the Zimmerwald SLR station, Switzerland. All the necessary parameters are defined for our own so-called point-like model which describes the motion of a point in space around the satellite centre of mass.