以太阳风为源水分子在月球空间环境中的分布特征

近年来,越来越多的观测结果均显示月球上存在水.本文通过运用Monte-Carlo方法及基于能量守恒的有心力场中粒子轨道算法对水分子在近月表的输运过程进行建模,得到了水分子在近月表分布随时间演化的图像.模拟结果显示,分布在高纬地区的水分子较同经度的中低纬地区要多,这与目前探测得到的结论是一致的.同时,对最终进入永久阴影区的水分子的百分比进行了统计,在光解离常数为6.4×10⁴s的情况下,有大约4.12%的水分子会被永久阴影区存储下来,这个比例与前人估算结果相吻合.     

基于递推自适应权重的快速稠密立体匹配

针对经典自适应权重稠密立体匹配算法计算量大的问题,提出了一种递推自适应权重算法.重新定义相邻像素的权重为距离衰减因子和色彩差异函数的乘积,不相邻像素权重为相邻像素权重的累乘,色彩差异越小、距离越近的像素权重越大;证明了在新的权重定义下,一维空间的匹配代价融合可以通过两次递推完成,真实图像的匹配代价融合可以通过4次递推完成,同时给出相应递推公式;递推匹配代价融合时每个像素每一视差只做4次乘法和8次加法,计算量比窗口大小为35×35的经典自适应权重算法小约两个数量级;基于递推匹配代价融合实现了一种快速稠密立体匹配算法.使用Middlebury大学的测评集测试该算法,证明了递推自适应权重算法的速度和精度均优于经典自适应权重算法.     

基于RT-LAB的组合导航仿真平台设计

设计了一种基于RT-LAB的SINS/GPS/CNS（Strapdown Inertial Navigation System/Global Positioning System/Celestial Navigation System）组合导航系统仿真平台方案,建立具有故障检测、隔离和系统重构能力的基于联邦卡尔曼滤波器的姿态、位置、速度组合导航系统方案和结构.将SINS与GPS的位置之差和速度之差作为SINS/GPS子滤波器的观测量,通过CNS给出的载体惯性姿态信息获得SINS的姿态误差角测量信息.仿真结果表明,该系统方案具有较强的容错性能、较高的导航精度和很强的实时性能,为组合导航技术的研究提供了有益的参考.     

A new design of low-power portable digital ionosonde

The Ionospheric Laboratory of Wuhan University is interested in upgrading its instrumentation replacing the WIOBSS (Wuhan Ionospheric Oblique Backscattering Sounding System) with a more flexible and automatic ionosonde. Then the updated ionosonde WMI (Wuhan Multifunctional Ionosonde) with automatic ionogram scaling has been developed to satisfy future research. The new system not only inherited some classic techniques from WIOBSS, such as the pulse compression and the coherent integration techniques, but also made great improvements in hardware design and software updating. This paper mainly introduces evolutions of this new ionosonde in both digital transceiver and digital signal processing domain, and also presents some observations.     

Dynamical evolution of high area-to-mass ratio objects in Molniya orbits

For special demands, some notable orbit types have been developed by human, including the Molniya orbits, which have a relatively high eccentricity up to about 0.7, and a period of 12 h. Considering that space debris with high area-to-mass ratio (A/M) has been discovered, such objects may also exist in Molniya orbits due to spacecraft and upper stages fragmentation events. However, there are not sufficient studies of the complex dynamical phenomena of such orbits. These studies can enrich the knowledge about the long-term evolution of these orbits, be helpful to propose uncatalogued objects observation and identification, and also set the protected region as well as active debris removal. In this paper, the characteristics of 2:1 resonance of Molniya satellite orbits are studied. A large set of numerical simulations, including all the relevant perturbations, is carried out to further investigate the main characteristics, and special attention is payed to the dynamical evolution of objects with high A/M, particularly affected by the direct solar radiation pressure. The long-term dynamical evolution of orbital elements, as well as the dependency of lifetime on the A/M value, is discussed.     

参数估计法在规则图形三维形貌测量中的应用

引入了参数估计法对规则图形三维形貌测量中的关键问题提高差分干涉系统横向定位准确度的方法进行了理论分析。仿真计算表明，在采用普通激光束径和工作台的条件下，系统横向定位准确度优于0.1μm，同时系统的复杂性和造价大大降低。     

基于目标一维距离像的雷达目标识别方法

讨论了马氏距离的性质,利用目标的一维距离像,提出了一种雷达目标识别方法.对雷达回波进行快速傅立叶变换,得到目标的一维距离像,计算其马氏距离,得到目标的稳定特征向量,根据相关算法进行目标识别.三种不同类型飞机回波的实测数据的识别结果,表明该方法是切实可行的.     

大速差射流燃烧室内三维湍流气固两相流的实验研究

本文用二维激光多普勒测速仪和探针取样法对大速差射流燃烧室中冷态三维湍流气固两相流动进行了实验研究,测量了气相速度,颗粒速度、颗粒质量流分布及两相各自的湍流特性,探讨了高速射流作用下两相流场的主要物理特征及其对火焰的稳定和强化燃烧的作用。     

亚音速、大攻角、时间域完全非定常机翼气动力的计算方法

 当前有关大攻角机翼气动力的数值方法,多数只适用于不可压情况。对于亚音速范围,只对定常情况进行过计算,至今尚未见到非定常方面的文章。为此,我们将文献[1]的方法作进一步发展,使之适合于计算大攻角非线性问题。由于亚音速非定常时间滞后以及尾涡形状不断变化,所以计算比较复杂,本文在处理过程中力求简单。