风速缺失情况下风电场功率调度分析

为了得到最优风电场功率调度方案,必须掌握任意时刻各风机风速输入值,进而得出各风机出力大小。当风速测量仪出现故障而不能正常工作时,风电机组风速数据将出现错误或缺失。建立线性回归方程,找出每台机组间输入风速的联系便可得到缺失的风速值。当风场发生“空转弃风”时,电网管理部门下达限电指令,风电场输出指定规模的有功、无功功率。将风场内所有双馈异步发电机损耗最低为目标函数,确定有功、无功调度方案。运用MATLAB软件建立风场模型,仿真结果验证了调度模型的可行性。     

方坯叶片电解加工过程的模糊控制方法

采集方料毛坯叶片电解加工整个过程的电流信号,用小波变换法对信号进行降噪处理,得到一条电流随间隙减小而呈增大趋势的光滑曲线。设计了一种二维M andan i型模糊控制器,以所得光滑电流曲线作为标准曲线,以加工电压的增量为模糊控制器输出,控制实际加工电流,使其在多种扰动下跟踪标准电流曲线。在M atlab的S im u link模块中,通过对由模糊控制器和电解加工系统组成的联合模型进行仿真试验,整定模糊控制器的3个增益参数。仿真试验表明,该方法可使电解加工系统较好地重现预设的加工过程,实现对电解加工全过程的控制。该方法也可以应用于其他类型的电解加工过程控制。     

非接触供电旋转超声加工系统负载特性研究

在旋转超声波加工过程中负载的变化会引起振幅衰减,进而造成加工精度和加工效率降低。本文针对非接触供电旋转超声加工系统在加工过程中振幅衰减的问题,首先,通过静态加载实验,获得了负载对超声振子电学参数的影响规律;其后,在此基础上进行了超声振子的非接触能量传输系统的加载实验,得到负载对能量传输特性的影响规律。实验结果表明,超声振子的电学参数受负载力大小、负载力方向和被加工材料特性的共同影响而发生改变,超声振子电参数改变引起了非接触供电超声系统输出功率的改变,进而导致了振幅衰减的问题;本文采用了串联谐振下主边串联电容、副边并联电容的电路补偿方式来减小振幅的衰减。本文的研究成果为解决振幅衰减问题提供了实验依据。     

稳态等离子体推力器羽流数值模拟

以国内研制的稳态等离子体推力器羽流为研究对象,建立了基于粒子单元法和直接蒙特卡罗模拟法的数值仿真模型,简化了电子动量方程,运用Boltzmann关系式求解了等离子体电势,研究了羽流电子数密度、离子电流密度及流场温度分布。通过与实验数据和已有数值结果对比,以验证模型和编制的程序。研究表明,羽流出口下游0.3~1.0 m处的羽流中心电子数密度约为2.5×1016~5×1015m-3,电流密度约为65~1 A/m2。文中工作对分析等离子体羽流污染具有参考意义。     

高速端面铣削加工引入残余压应力场的试验研究

为研究高速铣削加工表面残余应力分布,在统计试验设计指导下,使用X射线衍射/电解抛光方法对试样表层、次表层残余应力分布进行测量,得出残余应力分布曲线经验预报公式,探讨切削参数对残余压应力场特征指标的影响规律。研究结果表明,合理的高速切削工艺将在加工表面内引入类似喷丸强化效果的残余压应力场;(3,1)有理式模型与三阶多项式模型是描述高速铣削引入残余应力分布曲线的有效拟合公式;高速切削工艺参数对加工表面残余应力场的产生有直接影响,每齿进给量是决定残余压应力分布的关键因素,每齿进给量的变化将引起残余应力场形成机理的改变。     

钣金件快速精确加工中的激光切割工艺分析

针对δ0．5mm～δ6mm钣金件的结构特点,通过比较常用加工工艺和激光切割过程工艺．选出适合实际的优化方案。验证了不同切割参数对切割质量的影响。在工艺参数为：脉冲功率2．4kW、脉冲宽度约10ms、功率密度10^7W/cm^2的情况下,激光切割δ0．5mm～δ6mm钣金件获得了良好的切割质量,尺寸精度控制在误差（±100μm）范围内。工艺方案合理,生产率高。     

卫星垂直方向充退磁线圈设计新方法

文章提出采用电连接器对接安装方式设计卫星垂直方向充退磁线圈设备,可使卫星磁试验过程中去除吊装作业,大大提高其安全性。根据该思路进行线圈组位置布局及电性能参数的分析设计,然后完成充退磁线圈设备的结构设计和静力学有限元分析。在北京卫星环境工程研究所的CM2试验室内,研制完成的充退磁线圈设备已经在多颗卫星磁试验中获得很好地应用,它具有制造工艺简单、节省材料、操作安全方便等特点。     

Chatter stability and precision during high-speed ultrasonic vibration cutting of a thin-walled titanium cylinder

Titanium alloys are widely used in the aviation and aerospace industries due to their unique mechanical and physical properties. Specifically, thin-walled titanium (Ti) cylinders have received increasing attention for their applications as rocket engine casings, aircraft landing gear, and aero-engine hollow shaft due to their observed improvement in the thrust-to-weight ratio. However, the conventional cutting (CC) process is not appropriate for thin-walled Ti cylinders due to its low thermal conductivity, high strength, and low stiffness. Instead, high-speed ultrasonic vibration cutting (HUVC) assisted processing has recently proved highly effective for Ti-alloy machining. In this study, HUVC technology is employed to perform external turning of a thin-walled Ti cylinder, which represents a new application of HUVC. First, the kinematics, tool path, and dynamic cutting thickness of HUVC are evaluated. Second, the phenomenon of mode-coupling chatter is analyzed to determine the effects and mechanism of HUVC by establishing a critical cutting thickness model. HUVC can increase the critical cutting thickness and effectively reduce the average cutting force, thus reducing the energy intake of the system. Finally, comparison experiments are conducted between HUVC and CC processes. The results indicate that the diameter error rate is 10% or less for HUVC and 51% for the CC method due to a 40% reduction in the cutting force. In addition, higher machining precision and better surface roughness are achieved during thin-walled Ti cylinder manufacturing using HUVC.     

Characteristics of equatorial nighttime spread F – An analysis on season-longitude,solar activity and triggering causes

To understand global variability and triggering mechanisms of ionospheric nighttime equatorial spread F (ESF), we analyzed measurements from satellite and a ground-based GPS station for the years between 2010 and 2017. In this study we present seasonal-longitudinal as well as monthly variability of ESF occurrence for solar minimum and yearly variations of ESF occurrence for solar maximum and minimum periods. One of the long standing open questions in the study of ESF is what exactly initiates the Rayleigh-Taylor (RT) plasma instability growth. This question is the focus of the present work. Zonal background eastward electric field and E × B upward plasma drift speed patterns are found to be critically important in understanding plasma irregularity formation. In addition to particular patterns observed on these parameters, the background plasma density in the local evening hours just before the onset of ESF occurrence is very important. Stronger plasma densities just before the onset of irregularities resulted in stronger plasma irregularities, while relatively less dense plasma just before the onset of irregularities resulted in relatively lower plasma irregularities. Seasonal variations in ESF activity between March and September equinox seasons with comparable plasma densities can be defined in terms of the rate of change of solar flux F10.7 (dF10.7/day) index. Strongest ESF occurrence and strongest dF10.7/day are measured in the same month out of all other months in 2016 and 2017. Longitudinal variations of ESF activity in our measurements are related to longitudinal variations of plasma densities. We also found that ESF occurrence is better correlated with rate of change of F10.7 index for months in equinox seasons than for months in solstice seasons for the years between 2013 and 2016.     

Plasma electron temperature variability in lunar surface potential and in electric field under average solar wind conditions

The Moon is immersed in plasma environment. The most interesting challenge of the lunar plasma– field environment is that it is alternatively dominated by the extended but variable outer atmosphere of the Earth – the magnetosphere – and by the extended but highly variable solar atmosphere – the solar wind. Understanding the plasma environment and its interaction with the lunar surface will be beneficial to both manned and robotic surface exploration activities and to scientific investigations. Presented is a preliminary map of variations of lunar surface electric potential over the day side and night side using probe equations and a discussion on dust dynamics in this E-field structure using the data from Electron Reflectometer in Lunar Prospector spacecraft during 1998–1999. On the day side, potential is around 5 V and on the night side it reaches up to −82 V. On the night side region, only highly energetic electrons can overcome this large negative potential. The variation at electron temperature (T_e) strongly reflects in the surface potential. The potential reaches to a value of −82 V for T_e = 58 eV. Surface charging causes the electrostatic transport of charged dust grains. Dust grain size of 0.1 μm shows a levitation height of 4.92 m on lunar day side, 748 m on terminator region and 3.7 km on the night side. The radius of maximum sized grain to be lofted, R_max, peaks at the terminator region (R_max = 0.83 μm). At the transition region dust levitation is almost absent. This region is most suited for exploration activities as the region is free from hazards caused by lunar dust.