基于液相污染模型的航天器交会对接羽流污染研究

航天器交会对接任务一般由主动对接方和被动目标配合完成,交会对接飞行的主动寻的段和分离撤离段均可能出现主动对接方开启反向发动机进行反向紧急制动和撤离的情况,该情况下被动目标可能受到来自主动方反向发动机羽流污染影响。文章利用国际空间站羽流污染计算模型对交会对接任务羽流污染沉积进行了分析计算。     

基于独立桨距控制的电控旋翼主动振动控制

电控旋翼利用桨叶后缘襟翼偏转通过气弹作用带动桨叶变距,从而实现对旋翼的控制。但由于其系统的复杂性,桨叶间易存在扭转刚度和质量不相似,从而引起较严重的旋翼振动。针对该情况,提出了基于独立桨距控制的主动振动控制方法,并以某原理性电控旋翼为算例进行了数值仿真,验证了所提出控制方法对电控旋翼由扭转刚度和质量不相似引起振动的减振有效性,最佳减振水平可达90%。     

反台晶体及其应用

介绍了应用离子束刻蚀技术制作高基频反台晶体谐振器及反台晶体谐振器的应用。     

An ion analyzer for the lunar surface with E-parallel–B

We present a novel instrument concept to measure the energy and mass spectra of ions incident on the lunar surface, based on the E-parallel–B or Thomson-parabola device used extensively as a diagnostic in the plasma fusion community. The Apollo-era Suprathermal Ion Detector Experiment (SIDE) was the first instrument package to perform in-situ measurements of ions incident on the lunar surface. The ions can originate from a variety of sources, including the solar wind, the Earth’s magnetotail, and photoionization of the thin lunar atmosphere. The species and energy distribution of ions arriving at the lunar surface depend in a complicated and poorly-understood fashion on the phase of the lunar day, the position of the Moon with respect to the Earth, and on the local plasma environment.     

Ion engine grids: Function,main parameters,issues, configurations,geometries, materials and fabrication methods

Ion optics are crucial components of ion thrusters and the study of the different ion extraction solutions used since the beginning of the electric propulsion era is essential to understand the evolution of ion engines. This work describes ion engine grids' main functions, parameters and issues related to thermal expansion and sputter erosion, and then introduces a review of ion optics used for significant launched and tested ion thrusters since 1970. Configurations, geometries, materials and fabrication methods are analyzed to understand when typical ion thrusters use two or three grids, what are the thicknesses and aperture sizes of the screen, accelerator and decelerator grids, why molybdenum and carbon-based materials such as pyrolytic graphite and carbon–carbon are the best available options for ion optics and what is the manufacturing method for each material.     

Structure and kinetic properties of slow-mode shocks associated with magnetic reconnection in the near-Earth magnetotail

We study the structure and kinetic properties of slow-mode shocks near the plasma sheet boundary layer (PSBL) associated with magnetic reconnection by Cluster observation. The presence of slow-mode shocks is confirmed by traditional Rankine–Hugoniot (RH) analysis and Monte-Carlo shock fitting method. The Walén analysis, applied to the tailward flow associated with slow-mode shocks, also supports that plasma was accelerated across a Petschek-type slow-mode shock connected to the diffusion region. Back-streaming ions were observed on the shock layer, and cold ions were accelerated and heated by slow-mode shocks. In addition, whistler and electrostatic solitary waves were observed around the slow-mode shocks. These waves might be excited by the observed field-aligned electron beams near the shocks.     

Particle simulation of grid system for krypton ion thrusters

The transport processes of plasmas in grid systems of krypton (Kr) ion thrusters at different acceleration voltages were simulated with a 3D-PIC model, and the result was compared with xenon (Xe) ion thrusters. The variation of the screen grid transparency, the accelerator grid current ratio and the divergence loss were explored. It is found that the screen grid transparency increases with the acceleration voltage and decreases with the beam current, while the accelerator grid current ratio and divergence loss decrease first and then increase with the beam current. This result is the same with Xe ion thrusters. Simulation results also show that Kr ion thrusters have more advantages than Xe ion thrusters, such as higher screen grid transparency, smaller accelerator grid current ratio, larger cut-off current threshold, and better divergence loss characteristic. These advantages mean that Kr ion thrusters have the ability of operating in a wide range of current. Through comprehensive analyses, it can be concluded that using Kr as propellant is very suitable for a multi-mode ion thruster design.     

相对论性离子束（环束）流引起的电磁不稳定性

在相对论性框架下，研究了冷离子流产生的右旋共振模，非共振模电磁不稳定性的特征结果表明，非共振模不稳定性增长率受离子流初始参数影响较大，而右旋共振模的增长率则受离子流初始参数影响较小。此结果可应用于太阳高能离子流通过低日冕区和地球磁层辐射带俘获的高能质子情形。     

海尔-波普彗星离子尾的间断和波动

给出海尔-波普彗星近日点附近大尺度观测的结果.指出:1997年2月16、17和18日海尔-波普彗星等离子尾部分有断尾事件发生.观测时刻的离子尾内物质运动速度约为50km／s;离子尾射线向主尾主轴的并拢速度约为0.080'／s.1997年3月3日海尔-波普彗星离子尾有波动现象发生.波动发生在距离彗星密度中心约130×104km,偏离主轴30°处,振幅约20×104km、其离子束宽度约8×104km、波动的相速度约为200km／s.      

反作用控制系统推力器失效的外部检测与诊断

通过推进系统外部可测的姿态信息,利用强跟踪滤波器和多模预报估计器,研究了一类非线性系统常值阶跃型故障和间歇性故障的检测与分离问题。对关机失效,利用强跟踪滤波器获得故障效应的估计,检测逻辑采用改进的贝叶斯分类方法,依据推力器失效效应的方向性进行故障单元的分离;对开机失效,采用多模预报,根据相应残差向量范数的比较进行故障的即时无阈值判别,同时完成了故障后系统状态的重构问题。以一类大型航天器的反作用姿态控制系统为例,对其中出现的推力器失效进行了故障识别仿真研究,表明所提方法是有效的。