电源端口电磁脉冲防护方法研究

为了解决电源端口在不同电磁脉冲条件下的防护问题,提出了一种适用于多种电磁脉冲防护设计方法。该方法能依据不同电磁脉冲波形精准指导防护电路设计;该方法使用CST对电源端口电源线及电路建模进行仿真分析;利用其电磁仿真结果,设计防护电路;并采用数值计算方法对防护电路中的防护器件瞬态电压抑制器进行精准设计,可保证瞬态电压抑制器本身及后级电路不发生损坏,可为电源端口防护不同电磁脉冲提供理论依据。     

基于时频-小波分析的压气机失速过程研究

采用时频—小波分析的方法,针对某型发动机的八级轴流压气机级间压力信号,提取失速先兆及发展信息。结果表明,在失速前的阶段,不同的频率段表现出不同的失速先兆成分;并检验了失速时刻信号的奇异性,最后确定了最先失速级。      

永磁同步电机转子初始位置角在线检测方法

针对现有永磁同步电机(PMSM)转子初始位置角辨识方法存在的缺点,研究PMSM数学模型,推导电机转子位置与电机绕组电感之间的数学关系。提出利用电机三相绕组静态电感值初步判断转子位置,并用变频器发送激励电压实现转子的极性判断,进而准确辨识出转子的初始位置角。检测过程中无需转子预定位,且电机转子处于机械锁定或自由停止状态下均可实现。试验结果证明所提方法检测精度高,能够满足PMSM矢量控制的需求,具有一定的推广应用价值。     

小功率低速直驱笼型异步电动机研究

从机电一体化的角度提出了小功率低速直驱笼型异步电机(LLDSM)额定电压的确定方法,研究了额定电压与最大转矩倍数和变频电源最大输出电压之间的关系。论述了LLDSM极数和槽数的选择原则,并仿真分析了不同极槽配合时气隙磁场的谐波含量。最后对制作的LLDSM进行了试验,测得电机转矩与电流和电压的关系曲线,并对试验数据进行了研究分析,验证了理论分析的正确性。     

火电辅机变频器低压穿越直流电压补偿及其控制

针对火电辅机变频器因厂用电压跌落而触发闭锁,造成发电机组停机的问题,设计了基于变频器直流母线电压补偿的辅助穿越装置。辅机变频器采用直接转矩控制,低压穿越装置主电路采用三重交错并联升压变换器结构,在电压跌落期间维持变频器直流母线电压稳定,同时减小输出电流高频纹波。考虑到并联模块参数差异造成的均流问题,提出在传统电压电流双闭环控制的电压外环加入均流环的解决方法,消除环流,使开关管电流应力更为均衡。由于控制系统具有非线性、强耦合的特点,传统PI控制器存在局限性,所以利用模糊控制算法优化PI控制器参数整定,改善其性能。最后用仿真验证了所提方法的有效性。     

Ultraviolet spectroscopy of the extended solar corona during the Spartan 201 mission

The instruments on the Spartan 201 spacecraft are an Ultraviolet Coronal Spectrometer and a White Light Coronagraph. Spartan 201 was deployed by the Space Shuttle on 11 April 1993 and observed the extended solar corona for about 40 hours. The Ultraviolet Coronal Spectrometer measured the intensity and spectral line profile of HI Ly and the intensities of OVI 103.2 and 103.7 nm. Observations were made at heliocentric heights between 1.39 and 3.5 R. Four coronal targets were observed, a helmet streamer at heliographic position angle 135°, the north and south polar coronal holes, and an active region above the west limb. Measurements of the HI Ly geocorona and the solar irradiance were also made. The instrument performed as expected. Straylight suppression, spectral focus, radiometric sensitivity and background levels all appear to be satisfactory. The uv observations are aimed at determining proton temperatures and outflow velocities of hydrogen, protons and oxygen ions. Preliminary results from the north polar coronal hole observations are discussed.     

Coronal electron density measurements using the near-ir [Fe XIII] emission lines

Observations made during the 1991 total solar eclipse and recent observations from NSO/Sac Peak are discussed. The ground-based density measurements will be complimentary to SOHO observations, particularly SOHO electron density measurements.Operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation     

低速轴流压气机旋转失速特性试验

在一台双级低速轴流压气机上进行了均匀进气时的全流量特性试验研究,重点分析了该压气机旋转失速特性随流量系数的变化情况和失速起始特性.试验结果表明,压气机在失速前出现模态波扰动,其传播频率约等于40%转子旋转频率,范围贯穿整台压气机;压气机第二级在模态波扰动诱导下率先进入旋转失速,初始失速团旋转速度为83.3%转子转速;失速团在向第一级扩散传播过程中,其旋转速度逐步降低,最后稳定在41.9%转子转速;失速团旋转频率随着流量系数的降低而减小;失速团范围随着流量系数的减小而逐渐增加.      

Solar Wind Sources and Their Variations Over the Solar Cycle

In this paper I will briefly summarize the present status of our knowledge on the four different sorts of solar wind, their sources and their short- and long-term variations. First: the fast solar wind in high-speed streams that emerges from coronal hole regions. Second: the slow solar wind emerging from the non-active Sun near the global heliospheric current sheet above helmet streamers and underlying active regions. Third: the slow solar wind filling most of the heliosphere during high solar activity, emerging above active regions in a highly turbulent state, and fourth: the plasma expelled from the Sun during coronal mass ejections. The coronal sources of these different flows vary dramatically with the solar activity cycle.     

A Brief History of CME Science

We present here a brief summary of the rich heritage of observational and theoretical research leading to the development of our current understanding of the initiation, structure, and evolution of Coronal Mass Ejections.