离子推力器羽流场模拟以及Mo+CEX沉积分析

离子推力器工作产生的羽流会对航天器产生影响,严重时甚至会造成航天器无法正常工作,为了精确评估离子推力器羽流特性及其对航天器的作用,采用基于粒子轨道理论(PIC,Particle-In-Cell)的模型对复杂的航天器的离子推力器羽流进行了数值模拟,并结合最近几年发展起来的浸入式有限元(IFE,Immersed Finite Ele-ment),采用结构网格准确计算复杂边界电场。通过模拟,获得了Mo+CEX离子在卫星表面的最大可能沉积分布,定量分析了卫星表面Mo+CEX离子的最大可能沉积率,表明在垂直于推力器主束流方向的卫星组件的表面上容易产生较大的Mo+CEX离子污染沉积率,而平行于推力器主束流方向上Mo+CEX离子污染沉积率相对较小。     

考虑电荷交换的三维离子发动机栅极粒子模拟

为了对离子发动机光学系统进行数值分析，开发了考虑电荷交换的三维离子发动机栅极粒子模拟程序。模拟程序采用单元内粒子（PIC）方法，光学系统为双栅极结构，推进剂采用氙，总加速电压为1600V，栅极间距为1mm，粒子之间的电荷交换碰撞模型采用蒙特卡洛方法。采用链式存储结构存储粒子信息，可以实现数组式存储方法所不能实现的功能。使用粒子模拟程序对离子发动机光学系统进行了粒子模拟，模拟得到了栅极间的电场分布和氙离子空间分布。模拟结果表明，在所取工作参数下氙离子全部通过了栅极孔，未撞击到栅极上，验证了参数的合理性。     

电晕放电飘升机研究

基于B-B效应的电飘机是一种不对称电容器在高电压作用下产生推力的飞行器,由于它是一种无推进剂的飞行器而受到科技界的广泛重视。本文通过实验研究,分析电晕放电的特点,提出基于涡旋动力学理论的挠场与真空零点能相干原理来解释推力的产生。对B-B效应的深入研究将对航空航天的推进技术带来革命性的变化。     

基于带漂移的布朗运动的民用航空发动机实时性能可靠性预测

以民用航空发动机为研究对象,运用性能退化可靠性理论和随机过程方法,对发动机的可靠性进行了研究.通过分析发动机性能退化过程,建立了基于带漂移的布朗运动的可靠性模型,利用布朗运动特性研究了基于当前状态的退化时间预测方法,实例证明,该方法可操作性强,易于工程实现,为航空公司进行发动机机队科学管理提供了基础.      

用离子束辅助沉积(IBAD)工艺制备TiCxNy膜的研究

用离子束辅助沉积（ＩＢＡＤ）工艺在９Ｃｒ１８、ＧＣｒ１５钢基体上形成了ＴｉＣｘＮｙ膜。ＴＥＭ观察发现膜均呈多晶结构,都具有（１１１）、（２００）和（２２０）择优取向。ＡＥＳ和ＸＰＳ分析进一步证实,ＴｉＣｘＮｙ膜呈含氧配置。干摩擦表明膜的抗氧化性能优良,其存在能有效抑制基体在摩擦过程中氧化膜的形成。又由于膜的硬度高,润滑性良好,每种基体的磨损特性都得到了显著地改善。但随着基体不同,膜的力学机械性能随     

运动补偿用惯性器件误差对SAR成像分辨率的影响研究

 为提高合成孔径雷达（SAR）系统的性价比,必须根据SAR成像分辨率的要求和整体系统参数,设计相应精度的运动补偿用捷联惯导系统。在确定SAR运动补偿系统方案和安装方式的基础上,分析不同方向的加速度计和陀螺仪误差对天线相位中心位置测量误差的影响,并利用位置测量误差与SAR成像分辨率之间的关系,进一步明确了不同方向的加速度计和陀螺仪对SAR成像分辨率的影响。研究表明：基于SAR的工作原理和安装方式,x方向加速度计和y方向陀螺仪对SAR成像分辨率的影响明显比其他惯性器件严重;相同误差水平的惯性器件对SAR成像分辨率的影响随着合成孔径时间和工作波长的不同而不同,时间越长,波长越短,影响则越严重。SAR成像仿真证明了结论的正确性。研究结果对于研制高性价比SAR成像运动补偿系统有一定的理论指导意义。     

Statistical study of radio drifting pulsation structures with associated CMEs and other observations

Solar radio burst, especially the fine structures (FSs) and the drifting pulsation structures (DPSs), may be used as an important diagnostics tool to draw the evolution map of the flare loop in the initial phase of solar flares. In this work, 52 radio events were found accompanying with DPSs. They were all observed with the Solar Radio Spectrometers (0.625–7.6 GHz) of China during 1998–2004. Combining the radio observations with LASCO-C2, Goes-8 SXR, H_α, EUV and Trace observations, we analyzed all these events and obtained some statistic conclusions: First, 88% DPSs take place at the initial phase of the radio burst, and their rich spectrum characteristics are helpful to understand the events further. Second, 83% DPSs are associated with CMEs or ejection events, and all the events are accompanied by Goes SXR flare. Third, for CMEs and DPSs, which take the first step, there is no significant predominance of either of them. The relationship between the DPSs and CMEs is still not clear in this study because of the lack of spatial resolution in the centimeter–decimeter band. However, the EIT or Trace ejection happened during the onset/end time of DPSs. They are signatures of the initial phase of CMEs. Two events will be illustrated to explain this.     

Ion dynamics associated with Alfven wave in the near-Earth magnetotail: Two-dimensional global hybrid simulation

Ion dynamics in the near-Earth magnetotail region is examined during periods of fast Earthward flow with a two-dimensional (2-D) global-scale hybrid simulation. The simulation shows that shear Alfven waves are generated at x ∼ −10R_E, where the strong earthward flow is arrested by the dipole field, and propagate along field lines from the equator to both southern and northern polar ionosphere. Non-gyrotropic ion velocity distributions occur where the large-amplitude Alfven waves are dominant. The simulation indicates that the Alfven waves are generated by interaction of the fast earthward flow with the stationary near-Earth plasma. Beam ions are found to be pitch-angle scattered and trapped in the wave field, leading to the non-gyrotropic ion distributions in the high-latitude plasma sheet boundary. In addition, significant particle heating and acceleration are found to occur behind the dipolarization front due to the effect of wave turbulence.     

考虑侧风情况下的无人机自主导航控制技术研究

随着无人机应用范围的扩大,要求无人机能精确跟踪预定航线.介绍了无人机侧向导航控制律、切换准则和控制参数的限定;分析了侧风对无人机自主飞行时姿态的影响,以及在一种常用侧向控制律下形成侧风偏差的原因,给出了解决的办法.Matlab软件数字仿真的结果对比表明了控制系统抗侧风偏差的有效性.     

A 2-D comparison of ionospheric convection derived from SuperDARN and DMSP measurements

Ion drift vectors measured by the DMSP satellites are compared with plasma convection vectors obtained by the SuperDARN HF radars through the standard Map Potential algorithm of Ruohoniemi and Baker [Ruohoniemi, M., Baker, K.B. Large-scale imaging of high-latitude convection with super dual auroral radar network HF radar observations. J. Geophys. Res. 103, 20797–20811, 1998]. Despite significant data spread, the agreement can be qualified as reasonable for a data set comprising of 149 satellite passes over the Northern Hemisphere at high latitudes. The slope of the best-fit line relating SuperDARN and DMSP velocity magnitudes is of the order of 0.3 with a tendency for the SuperDARN velocities to be smaller. The agreement between the azimuths of the ion drift and convection is better with the slope of the best-fit line being close to 1. It is shown that consistency between the radar and satellite measurements is much better if the SuperDARN line-of-sight velocities are compared with the DMSP cross-track ion drifts for events showing slow spatial and temporal variations of the convection. If areas of strong convection changes are included into comparison, the degree of agreement deteriorates drastically. This result implies that differences in the spatial and temporal resolutions of DMSP and SuperDARN measurements are crucial factors contributing to the observed discrepancies. In addition, some differences are introduced when the SuperDARN line-of-sight velocities are filtered and reprocessed into vectors with the application of a background convection model.