结冰对民用飞机飞行性能的影响分析

在获取民用飞机适航合格审定证明前,必须通过飞行试验,并在试验中演示验证民用飞机能在CCAR25部附录C确定的连续和间断的最大结冰状态下安全运行。基于此背景,计算并得到某型机两种构型在45min待机冰型下的飞行性能,与无冰状态下对应构型的飞行性能进行对比分析。结果表明,结冰对飞机的飞行性能具有较大的影响。     

测控雷达伺服系统整流电路的建模与仿真

电力电子整流电路是测控雷达伺服系统的重要组成部分。某型测控雷达采用了三相零式反并联可逆整流电路结构。分析了整流电路可逆运行的工作原理以及晶闸管触发电路的控制方式,利用MATLAB/Simulink的建模功能,建立了触发脉冲产生电路和整流电路的模型,仿真得出系统可逆运行时电机的工作状态以及整流电路输出电压波形。仿真结果显示,此整流电路可以实现电机的四象限运行,所建模型正确。利用该模型可以对测控雷达伺服系统的分析和设计起到很好的辅助作用。     

机翼顶起设计解析

飞机全机顶起是飞机维护时必不可少的操作程序,其中机翼顶起是全机顶起的一个重要组成部分。机翼顶起设计包括两个方面内容,即顶垫设计和机翼千斤顶选型。顶垫设计与顶起点结构设计、机翼千斤顶选型是联合设计、相互影响的。     

A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind Simulations

It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.     

机型成本预测的因素分析法

根据管理会计把机型成本要素分解为固定成本、半变动成本和变动成本，对航空公司机型的航空运量作出预测，就可对机型作出预测。     

旋流器型式对空气雾化喷嘴雾化特性影响规律

采用试验与数值计算相结合方法研究了不同旋流器型式对双旋流式空气雾化喷嘴喷雾特性的影响规律.采用粒子图像测速(PIV)测量了不同空气雾化喷嘴下游流场结构,并且采用高速摄影仪和激光粒度分析仪,对不同空气流量和燃油流量下的双级旋流空气雾化喷嘴的油雾场形态、索太尔平均直径(SMD)、Rosin-Rammler分布进行试验研究;...     

点阵单元类型和排布角度对传热特性的影响

基于瞬态液晶测试技术和数值仿真,在相同孔隙率条件下,研究了桁架型点阵结构的单元类型和排布角度对矩形通道壁面对流传热特性的影响.结果表明:点阵单元类型对壁面传热性能有决定性的影响,其中交叉排布的体心立方(body centered cubic-0,BCC-0)和Kagome-0点阵归因于出色的传热强化效果,雷诺数在5 7...     

Investigating the Coronal Mass Ejections associated with DH type-II radio bursts and solar flares during the ascending phase of the solar cycle 24

We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric – hectometric (DH) type-II radio bursts (1–16?MHz) and solar flares during the period 2008–2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.We found that the events are mostly distributed around 15.32° and 15.97° at the northern and southern solar hemispheres, respectively. We found that there is a clear dependence between the longitude and the CME’s width, speed, acceleration, mass, and kinetic energy. For the CMEs’ widths, most of the events were HCMEs (～62%), while the partial HCMEs comprised ～35% and the rest of events were CMEs with widths less than 120°. For the CMEs’ speeds, masses, and kinetic energies, the mean values showed a direct proportionality with the longitude, in which the limb events had the highest speeds, the largest masses, and the highest kinetic energies. The mean peak flux of the solar flares for different longitudes was comparable, but the disk flares were more energetic. The intermediate flares were considered as gradual flares since they tended to last longer, while the limb flares were considered as impulsive flares since they tended to last shorter.A weak correlation (R?=?0.32) between the kinetic energy of the CMEs and the duration of the associated flares has been noticed, while there was a good correlation (R?=?0.76) between the kinetic energy of the CMEs and the peak flux of the associated flares. We found a fair correlation (R?=?0.58) between the kinetic energy of the CMEs and the duration of the associated DH type-II radio bursts.     

激光动态液位测量技术研究

如今,运载火箭大量使用液氧、煤油等液体推进剂,其液位测量技术主要有浮子式、激光式、电容式、雷达式等。介绍并实现了一种激光液位测量系统,该系统体积小、功耗低,可适应多种测量环境,能满足航天燃料液位测量高精度、高动态、连续稳定测量的要求。系统利用相位式激光测距技术,通过测量激光回波信号的相位延迟,计算激光光程从而得到距离数据并通过客户端进行直观展示和数据存储。系统最大测量距离可达100 m,精度为±1 mm。该系统为非接触测量,耐腐蚀,通过加入反射板可实现透明、非透明液体测量。     

副翼配重的着陆冲击响应

提供了一个计算副翼配重着陆冲击响应的方法。由于主起落架为纯摇臂式,考虑机体的弹性,机体和主起落架运动联立求解的加速度不是显式,因此必须用高斯方法解加速度的线性方程组,再用吉尔方法解微分方程。