LYAPUNOV-TYPE STABILIZATION FOR NONLINEAR UNCERTAIN SYSTEMS AND NONLINEAR H~∞ CONTROL

ＬＹＡＰＵＮＯＶ┐ＴＹＰＥＳＴＡＢＩＬＩＺＡＴＩＯＮＦＯＲＮＯＮＬＩＮＥＡＲＵＮＣＥＲＴＡＩＮＳＹＳＴＥＭＳＡＮＤＮＯＮＬＩＮＥＡＲＨ∞ＣＯＮＴＲＯＬＦｅｉＳｈｕｍｉｎ（ＲｅｓｅａｒｃｈＩｎｓｔｉｔｕｔｅｏｆＡｕｔｏｍａｔｉｏｎ，ＳｏｕｔｈｅａｓｔＵ...     

基于任务科目的直升机飞行品质评定试飞技术研究

主要对ADS-33E中飞行品质评定的要求进行分析,从任务科目、响应类型和可用感示环境3个维度进行飞行品质的等级评定研究,提出了直升机飞行品质综合评定的试飞技术研究思路,并对某型号直升机的试飞结果和有关问题进行了初步分析。     

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;...     

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。     

片切磨削方法构造的自由曲面磨削支持系统

以操作者高效准确操作数控磨削中心为目的,开发了自由曲面磨削支持系统,进行了基于球头磨具的磨削中心基础研究。讨论了获得高精度曲面的加工要点,并提出了片切磨削方法。     

航空发动机燃烧室的现状和发展

论述了燃烧室设计中各项技术指标的相互制约,分析了第3、4代发动机燃烧室的技术特点和燃烧室设计及研究方法的新进展.较详细介绍了驻涡（TVC）、富燃-快掺混-贫燃（RQL）、双环腔预混旋流（TAPS）、多喷嘴单元体和陶瓷燃烧室,指出其适用性.主动燃烧控制中更为主要的是出口温度分布系数控制,长远研究应开发快速、灵敏、配置严格的油气管理系统.最后讨论了燃用液氢的可行性.建议应加快CCD与燃烧室目标设计相结合的研发过程.