Two dimensional simulation of amplitude modulated electron plasma waves

Highly modulated waves near electron plasma frequency with both parallel and perpendicular polarization have been observed near diffusion region at dayside and in the tail region. In this paper, two dimensional Particle-In-Cell (PIC) simulation was performed to study the possible generation mechanism of these modulated electron plasma waves. It is shown that weak beam instability could generate the modulated Langmuir wave and the ambient magnetic field plays an important role in the formation of modulation. When the weak beam has loss cone distribution, highly modulated upper hybrid waves are generated and propagate with large angle to the ambient magnetic field. The properties of these modulated waves are discussed and compared with observations.     

基于主基底分析的变量筛选

利用Gram-Schmidt变换,提出一种主基底分析方法.解释并证明了Gram-Schmidt变换所删除的信息量.给出"主基底"的定义及构造方法,并提出"净信息含量比"的概念,用以测度所选基底包含的信息.该方法能在原始数据信息损失尽可能小的前提下,排除所有的冗余变量以及变量集合中的重叠信息,得到一个正交的主基底,从而更有效地对大规模变量集合中的信息进行筛选.多角度的理论分析指出,主基底在尽可能多地携带原始变量信息的同时,还可保证样本点间的相似性改变最小.实际案例分析说明了该方法的合理性和有效性.      

基于WSR的维修大纲审定方法研究

审定是飞机维修大纲投入使用的必要条件。分析了维修大纲审定的必要性,对维修大纲审订工作进行了研究：提出了基于物理-事理-人理的维修大纲审定方法;给出了基于该方法的概念模型;建立了维修大纲审定的指标体系;最后给出了基于指标的维修大纲审定多层模糊综合评判算法,并针对某新型支线飞机维修大纲进行了审定评估,效果良好,为我国飞机维修大纲审定满足适航要求提供了一种有效途径。     

机电驱动机构的线性特性

为研究雷达导引头机电伺服系统中的机电驱动机构特性,引入扭转刚度,建立了永磁式直流伺服电机驱动机构的传递函数模型,给出了电机与负载刚性和弹性连接两种条件下的传递函数.用频域拟合获得实际系统的传递函数.结果表明:测试结果与理论分析一致.该法对机电伺服系统设计和分析有一定的参考意义.     

液体火箭发动机试验频率量信号的处理与仿真

液体火箭发动机试验中频率量（流量、转速）数据曲线不规整,存在着“毛刺”。影响了数据的准确性。采用仿真方法优化频率量信号采集模式,并用实际试验数据进行了验证。结果表明,仿真方法优化频率信号采集模式能有效地减少频率量曲线中的“毛刺”。     

低雷诺数下翼型前缘流动分离机制的研究

采用高精度有限差分格式,对来流雷诺数为1.0×104,攻角为3°的二维翼型流动进行了直接数值模拟,研究了低雷诺数下翼型前缘流动的分离机制,描述了分离涡系的相互作用规律.计算结果表明:前缘椭圆弧靠近叶身位置存在吸力峰,流动在吸力峰内强逆压梯度的作用下发生分离;翼型上表面形成了包含驻留涡、脱落涡和二次涡的涡系结构,其尺度随时间不断变化,具有强烈的非定常性;表面压力分布曲线可以较好的描述翼型边界层流动.      

基于TSC MMS的远控精密测频系统设计

在高精度信号源测量中,由于Symmetricom公司的多通道相位测量设备TSC MMS（Multi-channel Measurement System）仪器自身功能限制,使得测量过程复杂繁琐,不利于操作。本文基于TSC MMS,利用网络实现远程控制与监测,设计用于精密频率源远程监测和性能测试的高精度时间频率测量系统。同时,扩展其功能,实现测量实时化、自动化,图形化。     

Changes in operational procedures to improve spaceflight experiments in plant biology in the European Modular Cultivation System

The microgravity environment aboard orbiting spacecraft has provided a unique laboratory to explore topics in basic plant biology as well as applied research on the use of plants in bioregenerative life support systems. Our group has utilized the European Modular Cultivation System (EMCS) aboard the International Space Station (ISS) to study plant growth, development, tropisms, and gene expression in a series of spaceflight experiments. The most current project performed on the ISS was termed Seedling Growth-1 (SG-1) which builds on the previous TROPI (for tropisms) experiments performed in 2006 and 2010. Major technical and operational changes in SG-1 (launched in March 2013) compared to the TROPI experiments include: (1) improvements in lighting conditions within the EMCS to optimize the environment for phototropism studies, (2) the use of infrared illumination to provide high-quality images of the seedlings, (3) modifications in procedures used in flight to improve the focus and overall quality of the images, and (4) changes in the atmospheric conditions in the EMCS incubator. In SG-1, a novel red-light-based phototropism in roots and hypocotyls of seedlings that was noted in TROPI was confirmed and now can be more precisely characterized based on the improvements in procedures. The lessons learned from sequential experiments in the TROPI hardware provide insights to other researchers developing space experiments in plant biology.     

大尺度弱纹理场景下多源信息融合SLAM算法

为实现自主机器人大尺度弱纹理场景下局部精准和全局无漂移的状态估计,提出一种视觉惯性与全球导航卫星系统多源信息融合的同时定位与地图构建算法。首先,通过在局部状态估计中加入线特征来更直观表示环境的几何结构信息,有效提升了弱纹理场景中关键帧之间相对位姿估计的准确性;其次,通过引入线性误差表示,将线性特征表示为直线端点上的线性约束,从而将线特征整合到基于特征点算法的线性表示中,有效改善算法在重复线特征场景下的鲁棒性。最后,使用多源信息融合算法,融合视觉惯性与GNSS测量信息实现了局部精确和全局无漂移的位姿估计,有效解决了大尺度弱纹理场景下的精准状态估计问题。多个公共数据集的评估结果表明,所提出算法的鲁棒性更强、定位准确度更高。     

Upstream of Saturn and Titan

The formation of Titan??s induced magnetosphere is a unique and important example in the solar system of a plasma-moon interaction where the moon has a substantial atmosphere. The field and particle conditions upstream of Titan are important in controlling the interaction and also play a strong role in modulating the chemistry of the ionosphere. In this paper we review Titan??s plasma interaction to identify important upstream parameters and review the physics of Saturn??s magnetosphere near Titan??s orbit to highlight how these upstream parameters may vary. We discuss the conditions upstream of Saturn in the solar wind and the conditions found in Saturn??s magnetosheath. Statistical work on Titan??s upstream magnetospheric fields and particles are discussed. Finally, various classification schemes are presented and combined into a single list of Cassini Titan encounter classes which is also used to highlight differences between these classification schemes.