多电飞机主发电机供电条件模拟装置设计

多电飞机主发电机要接入电网向电网供电,须要满足很多条件。首先要使准备接通的发电机励磁,然后当发电机转速正常,发电机电压达到要求后,并在外电源已经断开的条件下,接通发电机接触器,使发电机向电网供电。设计基于C8051单片机及外围电路的装置,对多电飞机主发电机接入电网的控制条件进行模拟,并将结果显示在装置的LCD(Liquid Crystal Display,简称LCD)显示屏上。该装置的设计包括硬件电路设计和软件程序编写。最后对装置进行调试与验证,实验结果能够达到设计初衷。     

Fundamental (f) oscillations in a magnetically coupled solar interior-atmosphere system – An analytical approach

Solar fundamental (f) acoustic mode oscillations are investigated analytically in a magnetohydrodynamic (MHD) model. The model consists of three layers in planar geometry, representing the solar interior, the magnetic atmosphere, and a transitional layer sandwiched between them. Since we focus on the fundamental mode here, we assume the plasma is incompressible. A horizontal, canopy-like, magnetic field is introduced to the atmosphere, in which degenerated slow MHD waves can exist. The global (f-mode) oscillations can couple to local atmospheric Alfvén waves, resulting, e.g., in a frequency shift of the oscillations. The dispersion relation of the global oscillation mode is derived, and is solved analytically for the thin-transitional layer approximation and for the weak-field approximation. Analytical formulae are also provided for the frequency shifts due to the presence of a thin transitional layer and a weak atmospheric magnetic field. The analytical results generally indicate that, compared to the fundamental value ($\omega =\sqrt{\mathit{gk}}$), the mode frequency is reduced by the presence of an atmosphere by a few per cent. A thin transitional layer reduces the eigen-frequencies further by about an additional hundred microhertz. Finally, a weak atmospheric magnetic field can slightly, by a few percent, increase the frequency of the eigen-mode. Stronger magnetic fields, however, can increase the f-mode frequency by even up to ten per cent, which cannot be seen in observed data. The presence of a magnetic atmosphere in the three-layer model also introduces non-permitted propagation windows in the frequency spectrum; here, f-mode oscillations cannot exist with certain values of the harmonic degree. The eigen-frequencies can be sensitive to the background physical parameters, such as an atmospheric density scale-height or the rate of the plasma density drop at the photosphere. Such information, if ever observed with high-resolution instrumentation and inverted, could help to gain further insight into solar magnetic structures by means of solar magneto-seismology, and could provide further insight into the role of magnetism in solar oscillations.     

Observation of a 27-day solar signature in noctilucent cloud altitude

Previous studies have identified solar 27-day signatures in several parameters in the Mesosphere/Lower thermosphere region, including temperature and Noctilucent cloud (NLC) occurrence frequency. In this study we report on a solar 27-day signature in NLC altitude with peak-to-peak variations of about 400?m. We use SCIAMACHY limb-scatter observations from 2002 to 2012 to detect NLCs. The superposed epoch analysis method is applied to extract solar 27-day signatures. A 27-day signature in NLC altitude can be identified in both hemispheres in the SCIAMACHY dataset, but the signature is more pronounced in the northern hemisphere. The solar signature in NLC altitude is found to be in phase with solar activity and temperature for latitudes $?70°$N. We provide a qualitative explanation for the positive correlation between solar activity and NLC altitude based on published model simulations.     

基于等效时间的混合储能系统高功率密度优化配置

越来越多的电力电子装置应用到多电飞机（MEA）电力系统中,导致MEA用电负荷功率呈现脉动特性,采用混合储能系统（HESS）平抑负荷功率脉动。为减少HESS重量,提出了一种高功率密度的优化配置方法。为建立负荷功率与储能介质之间的关系,提出了等效时间（ET）的概念,比较两者的ET常数作为储能系统类型选取的依据。进一步提出空间矢量法,采用能量型储能介质矢量和功率型储能介质矢量合成负荷功率,确定最优单体和截止频率,实现了HESS高功率密度配置。同时,从能量约束和功率约束两个方面进行HESS的容量的计算。最后,通过算例配置和仿真分析验证了本文所提方法的可行性和正确性。     

一种空间超大型可展开柔性聚光器

面向空间太阳能电站（SSPS）对大口径太阳能聚光器的应用需求,提出一种超大型、轻量化、高精度的空间可展开柔性聚光器的新构型。采取理论建模、计算仿真、优化设计相结合的方法对其抛物面构型原理、展开机构折展原理、展开态结构稳定性、动态聚焦精度等问题进行研究,并完成大口径可展开柔性聚光器的设计。提出了基于多层弹性花瓣镜体复合结构的大口径柔性聚光器优化创新设计方法。由于采用薄板柔索结构,本聚光器具有精度高、展收体积比大、质量轻、在线控制简单等优点,为空间太阳能电站千米级聚光器提供一种创新设计方法。     

串联式TBCC发动机风车冲压模态性能模拟

建立了基于部件低转速特性匹配的串联式涡轮基组合循环（TBCC）发动机风车冲压模态性能计算模型,提出了压气机低转速大流量特性扩展方法,由换算扭矩代替等熵效率表示旋转部件特性,解决了低转速部件效率不连续相关问题。分析了冲压外涵面积变化和涡轮功率提取对风车冲压模态性能及部件匹配的影响规律,并基于推力、流量连续准则设计了涡轮模态至冲压模态转换过程（含风车冲压模态）的参数调节规律。计算结果表明:在风车冲压模态下,冲压外涵面积变化对风扇工作状态有显著影响,对压气机影响较小;涡轮可提取功率随着风车转速的减小先增加后降低,比冲随提取功率的增加基本呈线性降低趋势,功率提取位置（高、低压涡轮）对部件匹配有显著影响。      

不平衡激励作用下周向加肋机匣振动能量传递机理

为了研究周向加肋机匣对整机振动的抑制机理,采用有限元法建立了加肋机匣-支承-转子耦合结构,结合振动功率流法分析了在转子不平衡激励作用下周向加肋机匣中的振动能量传递机理。 结果表明:机匣周向加肋筋诱导出的能量涡流场能够分流和耗散掉部分由转子传递至机匣的振动能量;机匣周向加肋筋改变了振动能量的传递路径,减小了机匣与支板连接处振动能量的回流现象;振动能量传递到机匣周向加肋筋后发生传递波波形的转换,携带大部分振动能量的弯曲波转换为纵波并沿加肋筋周向传递,阻断振动能量沿轴向传递至整机其他部位。 研究结果可为航空发动机结构设计以及整机减振提供参考。      

基于改进控制策略与动态无功支撑相结合的高电压穿越方法研究

针对双馈风力发电机高电压穿越问题,利用Laplace变换对电网电压骤升时电磁暂态过渡过程进行分析,得出定子电流不仅含有直流分量,还包含有工频交流成分,并通过仿真频谱验证了理论分析的正确性。不同于常规研究中只在转子电压方程考虑定子磁链的动态变化,而忽略了其对功率外环的影响,分析了定子磁链动态变化对有功、无功解耦的影响,在此基础上对功率外环进行传统矢量控制策略的改进。此外,考虑并网规范对机组无功电流支撑的要求,控制换流器输出与电网电压骤升幅度相匹配的无功电流,帮助故障电网快速恢复。仿真结果表明,该方案不仅能够保证电网电压骤升时双馈机组不脱网运行,而且也满足并网规范对机组无功电流输出的要求,实现高电压穿越。     

电容均压三相四开关变换器预测功率控制

三相四开关变换器直流侧分离电容电压不平衡,将降低其并网电能质量,缩短电解电容寿命。针对该问题,提出了一种直流侧分离电容电压均衡的模型预测功率控制策略。基于αβ两相静止坐标系分析电压矢量,建立功率预测模型。由于直流侧电容中点电压偏差值含有交流分量和直流分量,使用低通滤波器提取直流分量后计算功率补偿值,并计入给定功率,进行模型预测功率控制,实现直流侧分离电容电压均衡。该控制策略无需锁相环和PWM调制,易于实现。通过仿真和试验对其动、静态特性进行分析,验证了所提出控制策略的有效性和可行性。     

Attitude determination of planetary exploration rovers using solar panels characteristics and accelerometer

In this study, we propose a new attitude determination system, which we call Irradiance-based Attitude Determination (IRAD). IRAD employs the characteristics and geometry of solar panels. First, the sun vector is estimated using data from solar panels including current, voltage, temperature, and the normal vectors of each solar panel. Because these values are obtained using internal sensors, it is easy for rovers to provide redundancy for IRAD. The normal vectors are used to apply to various shapes of rovers. Second, using the gravity vector obtained from an accelerometer, the attitude of a rover is estimated using a three-axis attitude determination method. The effectiveness of IRAD is verified through numerical simulations and experiments that show IRAD can estimate all the attitude angles (roll, pitch, and yaw) within a few degrees of accuracy, which is adequate for planetary explorations.