基于黎曼距离的编队飞行卫星姿态控制系统故障检测数据优选方法

为突破星上资源的严苛约束、提升编队飞行卫星故障检测能力,提出了一种适用于编队飞行卫星姿态控制系统的故障检测数据优选方法,通过利用黎曼距离衡量无故障情况和故障情况下系统测量信息之间的差距,构建了编队飞行卫星姿态控制系统故障检测能力的评价指标。在此基础上,提出了故障检测数据优选方法,为系统输出信息结构优化提供了理论依据。仿真表明,所提出的方法能够在星上资源受限的情况下有效提升编队飞行卫星姿态控制系统的故障检测能力。     

基于APP的卫星地面遥控系统安全性设计

目前,我国绝大部分卫星的遥控指令上行操作必须在专用测控网内进行,当卫星发生在轨异常时,相关支持人员必须赶赴测控中心现场进行集中处置,非工作时段时效性较低,不利于紧急情况下的异常快速处置。对基于APP的卫星地面遥控系统安全应用方案进行了研究和设计,旨在为我国未来卫星高效运行管理提供一种新的手段,通过原型系统的仿真测试,验证了系统的技术可行性,实现卫星管理相关人员在远离测控中心的情况下也能安全有效地参与在轨异常应急处置。     

大涡模拟模型环形燃烧室污染特性

在任意曲线坐标系下,采用大涡模拟模型环形燃烧室两相燃烧流场中污染物的生成.用亚网格涡破碎(EBU)燃烧模型估算化学反应速率;分别用NO亚网格动力学模型与CO亚网格模型来模拟NO和CO的生成;采用随机离散模型模拟气液两相湍流流动,两相之间耦合采用PSIC算法.计算结果与瞬态速度场、出口温度和污染物质量分数分布的实验数据比较吻合,表明大涡模拟方法和亚网格模型可以用来预估实际燃烧室两相喷雾燃烧流场和污染物生成过程.      

合成孔径雷达卫星构型设计

合成孔径雷(Synthetic Aperture Radar,简称SAR)卫星的构型与其它卫星相比具有一定的特殊性,主要体现在大面积的相控平面SAR天线在工作时需侧视(长度方向沿飞行方向)和SAR天线与太阳电池阵之间的相容性.通过分析SAR卫星构型的特点,根据卫星构型设计的原则,结合SAR卫星的构型实例,给出SAR卫星构型设计的基本思路和方法.     

导航卫星中断频次的分析方法

面向导航卫星中断频次的定量分析需求,该文分析导航卫星中断产生的主要原因,给出中断频次分析的流程,并针对分析过程中的三个关键问题,研究提出具体实施方法,包括通过相关性分析快速定位底层中断事件,通过中断树建立指标分析模型,并融合在轨数据、地面试验数据快速预估得到底层功能异常率等。最后通过示例进一步说明中断频次分析过程。该文方法已应用于北斗导航卫星工程。     

空间绳系编队的动力学及稳定展开控制研究

以三角构型的空间绳系编队系统为对象开展了动力学特性分析和稳定展开控制研究。首先，针对以往编队动力学建模的精度问题，采用Lagrange法建立了系统动力学模型，建模时充分考虑了系绳的弹性，可在不增加计算量的同时保留系统的弹性特性。其次，根据所建立的动力学模型，定量分析了编队自旋稳定时自转角速度的范围，为之后的稳定展开控制提供理论依据。由于受制于执行机构精度和控制输入的限制，空间绳系编队系统是一个典型的欠驱动系统，采用分层滑模实现编队的稳定展开控制，仿真结果验证了该控制方法的有效性。     

Ionospheric parameters in the European sector during the magnetic storm of August 25–26, 2018

Variations of ionospheric parameters Total Electron Content (TEC) by GNSS, critical frequency (foF2) by vertical sounding and electron density (Ne) by low-altitude satellite were studied at high, mid and low latitudes of the European sector during the magnetic storm of August 25–26, 2018. During the main phase of the storm the ionospheric F2-layer was under the positive disturbance at mid and low latitudes. Then the transition from the positive to negative ΔfoF2 values occurred at all latitudes. The recovery phase was characterized by negative ionospheric disturbance at all latitudes. This is due to the decrease of thermospheric O/N2 ratio during the recovery phase of the storm. The intense Es layers screened the reflections from the F2-layer on August 26th at high and at low latitudes but at different times. Some blackouts occurred due to the high absorption level at high latitudes. In general, foF2 and TEC data were highly correlated. The major Ne changes were at the low latitudes. In general, Ne data confirmed the ionospheric dynamics revealed with foF2 and TEC.     

Estimating sea level rise around Australia using a new approach to account for low frequency climate signals

Regional sea level studies help to identify the vulnerable areas to the sea level rise. This study investigates the impact of climate modes on sea level variations and trends around Australia using altimetry data, climate indices, and sea level records from tide gauge stations. Here, we show that the sea level variations are negatively correlated with climate indices to the north and west of Australia. The spectral analyses of the climate indices and tide gauge data suggest that a low frequency signal with a period of 11 years emerges during the mid 1980s. Since the 25-year length of the satellite altimetry record is yet too short to detect low frequency signals, their effect on the estimation of regional sea level trend is unknown. Therefore, we estimate the sea level trend with consideration of this signal and using a two-step method. All signals with periods shorter than 7.5 years are first removed from sea level time series and then the trend is estimated using the parametric model that includes the 11-year signal. The skill of the parametric model in explaining the variations in sea level anomaly validates the presence of the 11-year signal detected in the spectrograms of the tide gauge data and climate indices. The average sea level trend for the study area is estimated as 3.85 ± 0.15 mm/year.     

Satellite selection methods for multi-constellation advanced RAIM

The increased number of potential threat modes under multi-constellation advanced receiver autonomy integrity monitoring (ARAIM) requires an increase in the number of subsets and a correspondingly high computational load. A new satellite selection method based on integrity support message (ISM) parameters is proposed and compared with GDOP-based selection. The performance was tested on five days of data measurements from 21 multi-global navigation satellite system experiment (MGEX) stations distributed around the world, as well as simulation using the broadcast ephemeris. The results show that the proposed ISM-based satellite selection method is highly compatible with the baseline ARAIM. This method could reduce the computational times by about 60–70% quickly, with minimising vertical protection level (VPL) loss, which was consistently within 1 m, even a reduced VPL value in some epochs, and resulting in an improved availability. The simulation results were similar to the MGEX data. It appears that the application of ISM-based satellite selection can effectively reduce computational burden with a minimal impact on availability.     

Fast cooperative trajectory optimization and test verification for close-range satellite formation using Finite Fourier Series method

The process of formation reconfiguration for close-range satellite formation should take into account the risk of collisions between satellites. To this end, this paper presents a method to rapidly generate low-thrust collision-avoidance trajectories in the formation reconfiguration using Finite Fourier Series (FFS). The FFS method can rapidly generate the collision-avoidance three-dimensional trajectory. The results obtained by the FFS method are used as an initial guess in the Gauss Pseudospectral Method (GPM) solver to verify the applicability of the results. Compared with the GPM method, the FFS method needs very little computing time to obtain the results with very little difference in performance index. To verify the effectiveness, the proposed method is tested and validated by a formation control testbed. Three satellite simulators in the testbed are used to simulate two-dimensional satellite formation reconfiguration. The simulation and experimental results show that the FFS method can rapidly generate trajectories and effectively reduce the risk of collision between satellites. This fast trajectory generation method has great significance for on-line, constantly satellite formation reconfiguration.