SCI协议实时性的仿真研究

可扩展一致性接口 ( SCI)是 IEEE提出的一个协议标准 ,主要用于高速、低延迟的大规模集群系统。对 SCI协议的基本拓扑结构——环网进行了建模 ,在此基础上 ,对一个典型的 4节点环进行仿真 ,考察特定消息的网络延迟和网络负载的关系。仿真结果表明 ,SCI协议适用于对实时性要求较高的任务系统的互联     

无陀螺磁控小卫星的大角度姿态捕获研究

为了解决无陀螺磁控小卫星的姿态稳定和捕获问题,本文针对偏置稳定的主动磁控小卫星姿态控制平台,基于磁控力矩的时间累积作用效果等效卫星角动量增量的规律,设计了一种仅利用角度反馈的卫星大角度磁捕获控制律。通过仿真和卫星在轨实测的验证,证明该方法具有良好的收敛效果和鲁棒性,工程实现简单,可靠性高,适用于中低轨道的通信小卫星。     

利用双星系统确定载体姿态研究

提出一种基于优化方法的双星定姿算法 ,将载波相位观测作了适当的变形 ,得到适用于基于向量观测的姿态确定算法的问题形式 ,然后采用QUEST算法求解姿态。深入分析了定姿方差和基线布局对定姿精度的影响。计算机仿真结果表明 ,分析的理论定姿精度与统计定姿精度吻合 ,说明了算法的可行性 ,对于实际应用具有一定的指导意义。     

基于解耦三轴气浮台非线性模糊变结构的鲁棒控制

根据三轴气浮台非线性动力学模型,研究了一种基于解耦的模糊变结构控制方法。设计的控制器不仅避免了一般变结构控制中的抖振,而且具有实现简单、工程化容易的优点。仿真结果表明,该模糊变结构控制法对模型的不确定性和外来干扰有较佳的跟踪性能,其鲁棒性较优。     

基于模型误差确定卫星姿态的预测滤波算法

本文给出了一种高精度、鲁棒性强的实时姿态估计算法，即预测滤波算法。该算法利用星敏感器所提供的观测矢量，对运动学方程中由陀螺漂移造成的角速度模型误差进行一步预测，从而准确地估计卫星的运动姿态和角速度。预测滤波算法的良好性能已通过仿真测试得到了验证。文中进一步提出的修正算法，使滤波器的预测性能得到了改进。     

GPS作为航天器全能敏感器的前景Ⅱ

在上文的基础上，简要介绍目前国外正在研制的几种典型的ＧＰＳ导航和姿态确定系统，展望ＧＰＳ作为航天器全能敏感器的前景，提出我国开发ＧＰＳ空间应用领域的几点建议。     

航天器姿态滑模变结构控制系统的设计

给出了航天器三轴动力学和四元数姿态运动学方程。在分析滑模变结构控制的基本原理和设计方法的基础上，通过二次型最优法解出航天器姿态角速度与姿态角之间的函数关系，进而得到滑动平面。在此基础上，应用滑模变结构控制方法对航天器姿态控制系统进行了设计和仿真，并与PID控制系统进行了分析比较。仿真结果表明，滑模控制系统具有良好的动态品质和稳态性能，体现了变结构控制的突出优点，对系统摄动和外加干扰具有极强的鲁棒性和自适应性。     

Tetrahedral satellite formation: Geomagnetic measurements exchange and interpolation

This note presents a study of a four-satellite tetrahedral formation to collect, process, and exchange multipoint measurements of geomagnetic field in a near-polar orbit. The study is conducted as a series of numerical experiments based on simulated spacecraft orbits and corresponding geomagnetic field models output. The four satellites are assumed to move in near-circular orbits specifically chosen to maintain the tetrahedron quality. The satellites exchange their simulated magnetometers readings and the collected multipoint measurements are processed on board of any of them thus creating an instantaneous interpolated map of the geomagnetic field in the interior of the tetrahedron. Interpolation is carried out with the use of Kriging algorithms, known in geostatistics for capturing spatial correlation of the data and taking into account statistical properties of the interpolated variables. We propose a concept of a servicing formation, and analyze interpolation accuracy for different formation sizes. It is then discussed how the processed multipoint measurements can be provided as a service to other nearby satellites. Finally, we show that using the existing COTS magnetometers it is possible to obtain real-time interpolation data, which are more precise at a given point and time than a conventional onboard magnetic field model, thus ensuring better attitude determination routines performance in the serviced spacecraft.     

Performance improvement of real-time PPP ambiguity resolution using a regional integer clock

Obtaining reliable GNSS uncalibrated phase delay (UPD) or integer clock products is the key to achieving ambiguity-fixed solutions for real-time (RT) precise point positioning (PPP) users. However, due to the influence of RT orbit errors, the quality of UPD/integer clock products estimated with a globally distributed GNSS network is difficult to ensure, thereby affecting the ambiguity resolution (AR) performance of RT-PPP. In this contribution, by fully utilising the consistency of orbital errors in regional GNSS network coverage areas, a method is proposed for estimating regional integer clock products to compensate for RT orbit errors. Based on Centre National d’Études Spatiales (CNES) RT precise products, the regional GPS/BDS integer clock was estimated with a CORS network in the west of China. Results showed that the difference between the estimated regional and CNES global integer clock/bias products was generally less than 5 cm for GPS, whereas clock differences of greater than 10 cm were observed for BDS due to the large RT orbit error. Compared with PPP using global integer clock/bias products, the AR performance of PPP using the regional integer clock was obviously improved for four rover stations. For single GPS, the horizontal and vertical accuracies of ambiguity-fixed PPP solutions were improved by 56.2% and 45.3% on average, respectively, whereas improvements of 67.5% and 50.5% in the horizontal and vertical directions, respectively, were observed for the combined GPS/BDS situation. Based on a regional integer clock, the RMS error of a kinematic ambiguity-fixed PPP solution in the horizontal direction could reach 0.5 cm. In terms of initialisation time, the average time to first fix (TTFF) in combined GPS/BDS PPP was shortened from 18.2 min to 12.7 min. In view of the high AR performance realised with the use of regional integer clocks, this method can be applied to scenarios that require high positioning accuracy, such as deformation monitoring.     

Higher order ionospheric error correction in BDS precise orbit determination

The ionospheric error affects the accuracy of the Global Navigation Satellite Systems observation and precise orbit determination. Usually, only the first order ionospheric error is considered, which can be eliminated by the ionospheric-free linear combination observation. But the remaining higher order ionospheric error will affect the accuracy of observations and their applications. In this paper, the influence of the higher order ionospheric error have been studied by using the International Geomagnetic Reference Field 13 and the Global Ionosphere Maps model produced by the Center for Orbit Determination in Europe. Focus on ionospheric error, the experiment of paper at doy 302 in 2019, which show that the second order ionospheric error impacting BeiDou Navigation Satellite System (BDS) B1I and B3I observation is 6.3569 mm and 11.8484 mm, respectively. Whereas, the third order ionospheric error impacting BDS B1I and B3I observation is 0.1734 mm and 0.3977 mm, respectively. Due to the current measurement accuracy of BDS carrier-phase observation can reach 2 mm, the influence of high order ionospheric error on observation should be considered. For BDS precise orbit determination, the orbit overlapping results are indicated that its orbit accuracy can be improved approximately 5 mm with the higher order ionospheric error correction, which is also in agreement with the results of Satellite Laser Ranging in this work.