斜激波极值规律的边界层影响

采用边界层理论与斜激波/膨胀波精确算法，建立一种结合Eckert参考温度法和Illingworth-Stewartson变换法优势的边界层权重算法，用于研究超声速黏性楔面边界层位移厚度对斜激波极值规律的影响。分别应用层流Navier-Stokes方程和湍流Navier-Stokes方程的CFD解算器对边界层新模型进行了算例精度评估。在来流马赫数为1.2~2.4和楔面角为3°~20°的范围内，压强比的相对误差小于0.1%。计入层流与湍流边界层影响的理论模型研究表明，边界层影响使得最优马赫数增加；对于层流边界层，最优马赫数增量约为0.001 5~0.003 3；对于湍流边界层，最优马赫数增量约为0.002 8~0.006 1。     

一种新型的干扰识别与检测算法

在通信系统抗干扰中干扰的检测及识别是一种关键的技术。文章提出了一种新的干扰识别算法。首先,应用盲信号分离算法来分离传感器接收到的混合干扰信号。然后从干扰信号的高阶累积量中提取特征参数用作进行SVM分类时的特征向量。最后,用SVM作为分类器来对单音干扰、多音干扰及脉冲干扰进行分类识别。计算机仿真结果表明,当信噪比不低于5d B时本文算法有较高的识别率。     

Dynamics of a spacecraft and normalization around Lagrangian points in the Neptune–Triton system

The problem of a spacecraft orbiting the Neptune–Triton system is presented. The new ingredients in this restricted three body problem are the Neptune oblateness and the high inclined and retrograde motion of Triton. First we present some interesting simulations showing the role played by the oblateness on a Neptune’s satellite, disturbed by Triton. We also give an extensive numerical exploration in the case when the spacecraft orbits Triton, considering Sun, Neptune and its planetary oblateness as disturbers. In the plane a × I (a = semi-major axis, I = inclination), we give a plot of the stable regions where the massless body can survive for thousand of years. Retrograde and direct orbits were considered and as usual, the region of stability is much more significant for the case of direct orbit of the spacecraft (Triton’s orbit is retrograde). Next we explore the dynamics in a vicinity of the Lagrangian points. The Birkhoff normalization is constructed around L₂, followed by its reduction to the center manifold. In this reduced dynamics, a convenient Poincaré section shows the interplay of the Lyapunov and halo periodic orbits, Lissajous and quasi-halo tori as well as the stable and unstable manifolds of the planar Lyapunov orbit. To show the effect of the oblateness, the planar Lyapunov family emanating from the Lagrangian points and three-dimensional halo orbits are obtained by the numerical continuation method.     

基于DSM的航天器信息建模方法及应用

将设计结构矩阵（DSM）技术应用于航天器研制的设计流程建模和信息建模,能够清晰准确地描述航天器各设计活动之间的信息耦合关系。根据航天器设计过程中跨分系统集成和协同设计的具体教学与培训需求,开发了一种基于DSM进行建模的工具软件,可用于建立一个基于设计参数信息的集成设计系统。根据其内在耦合关联关系,可实现各个分系统、各个模块、各个学科的参数信息一致和动态关联更新。     

实施"新洛桑"人才模式探索顶岗实习运行机制

顶岗实习是高职院校实践教学体系的重要组成部分,是职业教育实现工学结合突出学生就业能力培养的有效途径.杨凌职业技术学院酒店管理专业实施"新洛桑"人才培养模式,构建工学结合课程体系,探索顶岗实习运行机制.重点阐述了"新洛桑"人才培养模式及其顶岗实习运行管理机制,以期提高实践教学的质量,培养高技能酒店管理人才.     

Use of the ASTER satellite images for evaluation of structural changes in the Popocatépetl volcano related to microseismicity

Mexico is one of the most volcanically active regions in North America. Volcanic activity in central Mexico is associated with the subduction of the Cocos and Rivera plates beneath the North American plate. Periods of enhanced microseismic activity, associated with the volcanic activity of the Popocatépetl volcano are compared with periods, during which the microseismic activity was low. We detected systematical changes in the number of lineaments, associated with the microseismic activity due to lineament analysis of a temporal sequence of high resolution satellite images of the Popocatépetl volcano, provided by the ASTER/VNIR instrument. The Lineament Extraction and Stripes Statistic Analysis (LESSA) software package was used for the lineament extraction. In the future it would allow develop a methodology for detection of possible elevation of pressure in volcano edifice.     

反舰导弹换装发动机鉴定飞行试验方案设计

反舰导弹飞行试验的一项重要工作是检验发动机的工作性能及其他设备的匹配等。基于贝叶斯理论,利用数据综合技术设计反舰导弹换装发动机鉴定飞行试验方案,提出了小样本情况下弹上设备的鉴定方法,可为其他弹上设备鉴定提供重要参考。     

GNSS接收机在探月三期中的应用研究

探月工程对飞行器导航系统的性能提出了更高要求,因而有必要研究GNSS(Global Navigation Satellite System,全球导航卫星系统)接收机在探月任务中的应用。以探月工程三期为应用需求,开展地-月-地转移过程中的GNSS接收机可用性分析、GNSS信号特性分析;并针对低信噪比环境下的高灵敏度接收机系统应用进行设计,采用弱信号捕获算法和弱信号跟踪算法实现-175dBW的灵敏度;最终采用基于轨道动力学模型的卡尔曼滤波方法实现了GNSS自主定轨算法。仿真表明:GNSS接收机在60 000km以下的地-月转移和月-地转移弧段能够为探月飞行器提供100m以内位置精度的导航服务。     

锚固站数量及布局对导航星座自主定轨影响分析

针对导航星座自主定轨中的星座整体旋转问题,采用增设少量地面锚固站的方法可有效解决该问题。通过推导星地距离对卫星轨道升交点赤经的偏导数,证明了星地距离对卫星轨道升交点赤经可观。仅考虑在我国大陆范围内布设锚固站的条件下,仿真分析了锚固站数量以及布局对导航星座自主定轨精度的影响。仿真实验结果表明:采用3个以上的锚固站,即可有效控制星座整体旋转,在14d的仿真时段内卫星自主定轨精度保持4m以内;锚固站数量越多,自主定轨精度越高,但随着锚固站数量的增加,自主定轨精度改善程度越来越小;在保持4个锚固站的情形下,采用不同的锚固站布局方案,自主定轨精度并无明显差别。     

3-连通无爪图的最长圈

Hamilton问题是图论中重要的问题之一,已经得到了很多很好的结果,但一个图是Hamilton图的充分必要条件到现在还没有得出,于是开始研究无向图的最长圈,文章应用幅度的概念,使用反证法,通过构造最长圈并得出矛盾的方法,给出了3-连通无爪图最长圈的下限 .