MEMS梳齿音叉陀螺温度漂移特性研究

由于MEMS音叉陀螺多用于车载及无人机导航等应用场合,而外界温度环境因素对其零偏性能有着很大的影响,因此其温度引起的零偏漂移的大小直接影响着最终导航的性能。研究了全温范围传感器漂移特性,旨在提升陀螺温度漂移特性。通过改进电路设计以及采用实时补偿算法对其全温范围温度引起的零偏漂移进行补偿,将零偏稳定性提升了一个数量级。     

基于足部安装MIMU的行人导航系统设计

针对无卫星环境中行人导航定位需求,设计了一种基于足部安装MIMU的行人导航系统,重点研究了行人导航鞋传感器选型及样机设计流程;并在此基础上设计了基于零速修正和航向修正的行人导航算法,研究了零速区间内最优航向角的提取方法,实现了对瞬时磁干扰产生的磁航向角的有效判断。最后,利用设计的行人导航系统开展了三维空间航迹测试实验,实验结果表明,在不增加高度约束的条件下,该行人导航系统定位精度为0.33%,能够满足坡路环境中行人的定位需求。     

基于Hough变换的直线检测

给出Hough变换的基本原理。针对图像空间的直线检测问题，提出基于Hough变换的检测算法。利用该算法进行计算机仿真，分析清零阈值和清零邻域的范围对检测结果的影响，并给出算法改进方向。     

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.      

地球静止轨道卫星电推进位保策略研究

研究了利用电推进系统进行GEO卫星轨道保持问题,给出了一种基于日预报的位置保持策略。首先,根据GEO卫星轨道漂移规律,分析了小推力推进系统每日进行位保的可行性;然后,针对四电推力器配置构型,给出了每日轨道误差、各推力器工作时间与区间的预测方法;进一步,针对给定的定点位置,根据位保效果对电推进安装角进行了优化选择,并研究了推力变化对位保效果和燃料消耗的影响。以东经100°定点为例对所给方法进行了仿真验证,数值结果表明:所给策略可有效用于GEO卫星位置保持。     

模型参考自适应原理在冲击信号零点偏移补偿中的应用

在对衬垫材料进行冲击特性的实验研究时，测量所获得的波形常含有零点偏移，零点偏移的存在将对实验结果相入不可忽略的误差。因而在数据处理时应首先对零偏进行补偿以提高测量精度。本文作者根据在实测波形特征分析和能量原理基础上所建立的补偿方法，将现代控制理论中的模型参考自适应原理用于冲击信号的零点偏移补偿，拟定了模型参考自适应算法，给出了参考模型的建模途径，并编制了应用软件，支实验数据进行零偏补偿，取得了满意     

USB系统多副载波调制对测距性能的影响

侧音测距是统一S频段(USB)系统中经常采用的测距方式。针对某型综合基带测试中出现的测距距离漂移过大的问题,首先对侧音测距的原理、多副载波调制信号的特性进行分析,然后通过实验测试论证,讨论在不同的调制度、调制数据、副载波频率和码速率组合情况下,多个副载波交叉调制产生的组合频率对测距主音的干扰,从而确定了问题产生的原因,最后根据理论分析和实验测试结果提出一些预防措施。     

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.     

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.