基于DTC的开关磁阻电机转矩脉动抑制方法研究

开关磁阻电机(SRM)具有诸多性能优势,发展前景广阔,然而严重的转矩脉动极大地限制了其应用范围.对SRM直接转矩控制方法(DTC)进行了研究,对DTC的核心思想进行了介绍,给出了空间电压矢量的选取原则.采用有限元法(FEM)和神经网络(NN)相结合的方法,在Matlab中搭建了一个四相8/6极SRM的动态仿真模型.在不同的工况下,对DTC的控制性能进行了仿真分析,结果表明,DTC的引入可以有效地抑制SRM的转矩脉动,同时保证系统具有良好的调速和带载能力.     

Plasma and electromagnetic wave simulations of meteors

Every day billions of meteoroids impact and disintegrate in the Earth’s atmosphere. Current estimates for this global meteor flux vary from 2000 to 200,000 tons per year, and estimates for the average velocity range between 10 km/s and 70 km/s. The basic properties of this global meteor flux, such as the average mass, velocity, and chemical composition remain poorly constrained. We believe much of the mystery surrounding the basic parameters of the interplanetary meteor flux exists for the following reason, the unknown sampling characteristics of different radar meteor observation techniques, which are used to derive or constrain most models. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. We present our results on meteor plasmas simulations of head echoes using particle in cell (PIC) ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body. We also present the results of finite difference time domain electromagnetic simulations (FDTD), which can calculate the radar cross section of the simulated meteor plasmas. These simulations have shown that the radar cross section depends in a complex manner on a number of parameters. These include the angle between radar and meteor entry, a large dependence on radar frequency, which shows that for a given meteor plasma size and density, the reflectivity as a function of probing radar frequency varies, but typically peaks below 100 MHz.     

Synthetic Environments for Simulated Missions

Synthetic environments offer Space Flight projects an opportunity to perform rapid, comprehensive, and rigorous modeling of the critical elements of a mission in order to compute quantitative measures of design performance, associated risk, and actual mission utility value. Significantly, these studies can be performed early in the mission cycle. These synthetic terrains are generated on parallel, high-performance computers and served to remote simulations at near-interactive speeds. The terrain creation uses a realistic sequence of physical phenomena such as cratering and dusting with parametric control of features such as surface roughness and rock density. Terrain resolution may be arbitrary but typically ranges from 0.01 to 10 meters. The terrain server has been used for two rover simulations, one using the actual Sojourner autonomy flight code, and the other a more general algorithm. Monte Carlo studies of rover designs interacting with synthetic environments were executed in parallel to quickly compute performance statistics and risk estimates.     

WIOBSS: The Chinese low-power digital ionosonde for ionospheric backscattering detection

The ionospheric laboratory of Wuhan University has developed an ionosonde over about seven years. The prototype is designed as a portable, low-power digital MF (medium frequency) and HF (high frequency) radio system with high range and Doppler resolution. The first system is used for ionospheric oblique backscattering detection and called WIOBSS (Wuhan Ionospheric Oblique Backscattering Sounding System). WIOBSS is a portable monostatic ionosonde for both ionospheric research and HF channel management, adopting alternate transmitting and receiving patterns to transmit long coded pulse trains for high pulse compression gain. The almost perfect sequences are applied to modulate the pulse train for sounding without range sidelobes and the echo phase is used to estimate the Doppler velocity and velocity fluctuation. This paper introduces the new techniques adopted by WIOBSS and presents some observations.     

挠性空间结构的H∞辨识

重点研究挠性空间结构的Ｈ∞辨识，研究表明：依据系统的输入输出空间，对系统的未知动力学参数估计和对高维数截断的适当操作，将导致适合于控制的低维数学模型。模型维数确定时，系统模型与实际系统的距离在Ｈ∞范数的意义下几乎为最小，模型维数足够大时，系统模型与实际系统的距离可任意小，这是文下间提出了挠性空间结构Ｈ∞辨识的基本思想，为此，以带挠性梁的卫星系统为背景，首先分析了系统的动力学特性，引入了挠性系统Ｈ∞     

A program to measure new energetic particle nuclear interaction cross sections.

The Transport Collaboration, consisting of researchers from institutions in France, Germany, Italy and the USA, has established a program to make new measurements of nuclear interaction cross sections for heavy projectiles (Z > or = 2) in targets of liquid H2, He and heavier materials. Such cross sections directly affect calculations of galactic and solar cosmic ray transport through matter and are needed for accurate radiation hazard assessment. To date, the collaboration has obtained data using the LBL Bevalac HISS facility with 20 projectiles from 4He to 58Ni in the energy range 393-910 MeV/nucleon. Preliminary results from the analysis of these data are presented here and compared to other measurements and to cross section prediction formulae.     

开放进化式切削数据平台的开发应用

自1964年10月美国金切联合研究公司建立了第1个金属切削数据库以来,世界各国相继建立了各种切削数据库.计算机技术的飞速发展促使人们对切削参数的选取提出了更高的要求,切削参数的数字化和共享化已经成为大势所趋.     

CAXA PLM构建型号研制设计工艺生产一体化数字平台

军工制造业的行业特征和信息化发展趋势 军工制造业是国家战略性产业,也是国家制造业的重要组成部分,它是指研制、生产武器装备(包括系统、整机、零部件等)和具有明显军工高技术特色主导产品的制造业的总称.     

KM6水平舱消防灭火系统介绍

消防灭火系统是KM6水平舱的重要组成系统之一。由于舱内环境的特殊性,使得该系统不同于普通的消防灭火系统。针对KM6水平舱舱内的特殊环境,本文章分析了消防灭火系统的关键问题,提出了解决的具体方案,结合目前国际上先进的消防灭火技术,设计提出了适合KM6水平舱特殊环境的消防灭火系统具体方案。系统经过调试后表明：该系统设计理念先进,能很好的地满足水平舱“人-船-服”联合试验的需要。