Ⅰ型极值分布的环境因子

本文通过对Ⅰ型极值分布的理论分析和环境因子的二因子法，分别得到了Ⅰ型极大值分布和Ⅰ型极小值分布的环境因子，它们与正态分布的环境因子^[1]具有相同的形式，对Ⅰ型极值分布的环境因子进行了点估计，提出了用环境因子进行数据转换和综合的步骤。     

Study of backward propagating Langmuir waves with PIC simulation

The conversion of Langmuir waves into electromagnetic radiations is an important mechanism of solar type III bursts. Langmuir waves can be easily excited by electron beam instability, and they can be converted into backward propagating Langmuir waves by wave–wave interaction. Generally, the backward propagating Langmuir waves are very important for the second harmonic emission of solar type III bursts. In this work, we pay particular attention to the mechanism of the backward propagating Langmuir waves by particle in cell (PIC) simulations. It is confirmed that the ions play a key role in exiting the backward propagating Langmuir waves. Moreover, the electron beam can hardly generated the backward propagating Langmuir waves directly, but may directly amplify the second harmonic Langmuir waves.     

民用飞机通用地面支援设备选型程序浅析

为了满足航空公司/维修单位高效率、低成本的要求,在飞机的设计过程中,尽量减少专用地面支援设备的种类,以通用地面支援设备取代,成为了飞机主制造商及其供应商共同努力的目标,也成为了一种发展趋势。因此,在飞机运营及维护、维修过程中,通用地面支援设备的选型及程序显得越来越重要。     

等离子体彗尾流线断裂现象的讨论

等离子体Ⅰ型彗尾流线的断裂,已多次被人们见到.本文用MHD的理论,讨论和分析了这种现象,认为这是一种空间等离子体扰动所产生的结果.本文作了定性的分析,及定量的计算,比较满意地解释了这种彗尾中的观测现象.      

基于Patran/Nastran 和Hypersizer的复合材料后机身加筋结构形式选择分析

针对复合材料后机身加筋壁板构型选择问题,采用有限元前后置处理软件Patran建立有限元模型,使用有限元分析软件Nastran进行初步分析,利用复合材料结构分析与优化软件Hypersizer进行结构形式的优化计算分析,优选出后机身壁板最佳结构形式。通过计算分析,得出有意义的工程经验。     

Height of shock formation in the solar corona inferred from observations of type II radio bursts and coronal mass ejections

Employing coronagraphic and EUV observations close to the solar surface made by the Solar Terrestrial Relations Observatory (STEREO) mission, we determined the heliocentric distance of coronal mass ejections (CMEs) at the starting time of associated metric type II bursts. We used the wave diameter and leading edge methods and measured the CME heights for a set of 32 metric type II bursts from solar cycle 24. We minimized the projection effects by making the measurements from a view that is roughly orthogonal to the direction of the ejection. We also chose image frames close to the onset times of the type II bursts, so no extrapolation was necessary. We found that the CMEs were located in the heliocentric distance range from 1.20 to 1.93 solar radii (Rs), with mean and median values of 1.43 and 1.38 Rs, respectively. We conclusively find that the shock formation can occur at heights substantially below 1.5 Rs. In a few cases, the CME height at type II onset was close to 2 Rs. In these cases, the starting frequency of the type II bursts was very low, in the range 25–40 MHz, which confirms that the shock can also form at larger heights. The starting frequencies of metric type II bursts have a weak correlation with the measured CME/shock heights and are consistent with the rapid decline of density with height in the inner corona.     

旋转弹导引头红外角跟踪回路研究

分析了导引头红外末制导角跟踪回路的稳态性能对旋转弹跟踪性能的影响,以及起伏噪声对制导精度的影响,提出了采用二阶无静差角跟踪回路的改进办法.针对改进后的角跟踪回路,计算出了失调角和目标视线角之间的关系,并采用卡尔曼滤波将目标视线角速度准确地估计出来.试验结果表明:二阶无静差系统可以提高旋转弹的跟踪性能,且能够输出满意的制导信号,具有很好的实用价值.     

基于信息管理与融合技术在目标类型识别上的研究

在系统模型的基础上结合实战提出影响目标飞机类型识别的证据,并按照影响程度进行优先权排序;结合数据库,提出证据概率计算的数学表达式;采用深度优先搜索的融合模式,按照D-S证据理论进行融合计算;在传感器管理模块的作用下,对融合结果进行反馈控制;结合实例,对系统进行仿真验证,证明其可靠有效。     

Relationships between energetic storm particle events and interplanetary shocks driven by full and partial halo coronal mass ejections

We have analysed energetic storm particle (ESP) events in 116 interplanetary (IP) shocks driven by front-side full and partial halo coronal mass ejections (CMEs) with speeds $>$400 km s^?1during the years 1996–2015. We investigated the occurrence and relationships of ESP events with several parameters describing the IP shocks, and the associated CMEs, type II radio bursts, and solar energetic particle (SEP) events. Most of the shocks (57 %) were associated with an ESP event at proton energies $>$1 MeV.The shock transit speeds from the Sun to 1 AU of the shocks associated with an ESP event were significantly greater than those of the shocks without an ESP event, and best distinguished these two groups of shocks from each other. The occurrence and maximum intensity of the ESP events also had the strongest dependence on the shock transit speed compared to the other parameters investigated. The correlation coefficient between ESP peak intensities and shock transit speeds was highest (0.73 $\pm$ 0.04) at 6.2 MeV. Weaker dependences were found on the shock speed at 1 AU, Alfvénic and magnetosonic Mach numbers, shock compression ratio, and CME speed. On average all these parameters were significantly different for shocks capable to accelerate ESPs compared to shocks not associated with ESPs, while the differences in the shock normal angle and in the width and longitude of the CMEs were insignificant.The CME-driven shocks producing energetic decametric–hectometric (DH) type II radio bursts and high-intensity SEP events proved to produce also more frequently ESP events with larger particle flux enhancements than other shocks. Together with the shock transit speed, the characteristics of solar DH type II radio bursts and SEP events play an important role in the occurrence and maximum intensity of ESP events at 1 AU.     

基于螺旋理论的环形桁架式可展天线构型综合

基于螺旋理论针对环形桁架式可展天线机构的构型综合问题进行研究，首先概述基于螺旋理论的约束综合法，然后分析环形桁架可展天线机构的收展原理，将环形桁架机构分为上下环形边两部分，通过综合环形边机构并连接上下环形边便可得到环形桁架机构；采用移动副(P)来描述各个节点花盘的运动特性，通过基于螺旋理论的约束综合法针对环形边支链机构进行分析与综合，得到了16种约束支链机构，通过分析与优选得到了两种约束支链机构；采用综合得到的约束支链机构组合得到了环形边链路机构并通过连接组合与推演得到了四种环形桁架可展开机构；最后针对综合得到的四种环形桁架机构在Solidworks软件中进行了三维建模与运动仿真，校验了各机构的可展性。本文的研究为可展天线机构的构型综合提供了一种新思路，综合得到的几种环形桁架机构在空间可展开天线领域具有较好的应用前景。