加筋板中超高速撞击声发射源定位方法

加筋板是航天器上的常用结构。为研制基于声发射技术的在轨感知系统,需要研究加筋板中声发射波传播规律及撞击源定位方法。文章测定了断铅信号在加筋板中的传播速度,对沿不同方向传播的波速进行了比较;通过有限元仿真,研究了筋体几何尺寸对板中声发射信号传播规律的影响。试验与仿真的结果表明:筋体对信号压缩波波速影响较小,但会造成信号第一幅值的衰减,在传感器布局设计时需要考虑到该因素。将加筋板中声发射信号传播速度取为沿不同方向传播波速的平均值,可将源定位问题转化成求取函数最小值的优化问题,在加筋板上对断铅波源和超高速撞击波源进行定位效果较好。     

一种大偏距埋入式进气道气动特性试验

对一种大偏距埋入式进气道进行了高速风洞试验研究,得到了该进气道的气动特性,结果表明:①巡航状态时,出口马赫数的变化对进气道性能影响不大,进气道具有较高的巡航性能.②在试验研究的范围内,随飞行马赫数的增加,进气道性能有所下降;攻角的增加对进气道性能有所改善,侧滑角的变化对进气道性能影响不大.③进/发匹配点时,进气道通道内气流脉动功率谱密度分布呈现白噪声特征,在大攻角或偏航条件下进气道气流脉动功率谱密度有明显的峰值.      

A300-600飞机前缘缝翼故障排除

介绍了A300—600飞机前缘缝翼系统的工作原理,对于航线维护中出现的典型故障进行了详细的分析,简述了故障的排除方法,给出了提高该系统可靠性的维护建议。     

导弹无线电引信电磁脉冲效应仿真

以LFM导弹无线电引信为研究对象,以Ansoft软件为仿真平台,建立无线电引信天线模型和电路模型,通过计算机仿真对高功率微波(HPM)干扰导弹无线电引信的效应进行了研究。仿真结果表明,在高功率电磁脉冲作用下,混频器和滤波器上分布的电压很高,而进入执行级的电压很低,达不到启动电压的幅度。     

高功率密度DC-DC模块电源设计与分析

通过对有源箝位单端正激变换器、平板变压器、热设计以及结构设计的分析与计算,详细介绍了高功率密度DC-DC模块的设计方案,并在此基础上成功研制了一款100 W DC-DC电源模块,其功率密度高达3.4 W/cm3。采用本方案有效解决了当前DC-DC电源模块小型化的关键问题。     

用于磁悬浮轴承的三电平PWM开关功放设计

三电平PWM开关功放是适用于磁悬浮轴承的新型放大器。本文简述了该放大器的工作原理,在此基础上设计了以FPGA为核心的功放电路。分别介绍了电路各部分组成,工作原理及设计中的注意事项。试验结果证明了此种功放在系统所需频率范围内具有良好的动态特性。     

Particle acceleration and gamma rays in solar flares: Recent observations and new modeling

Experiments on SMM, GAMMA, Yohkoh, GRANAT, Compton GRO, INTEGRAL, RHESSI and CORONAS-F satellites over the past three decades have provided copious data for fundamental research relating to particle acceleration, transport and energetics of flares and to the ambient abundance of the solar corona, chromosphere and photosphere. We summarize main results of solar gamma-astronomy (including some results of several joint Russian–Chinese projects) and try to appraise critically a real contribution of those results into modern understanding of solar flares, particle acceleration at the Sun and some properties of the solar atmosphere. Recent findings based on the RHESSI, INTEGRAL and CORONAS-F measurements (source locations, spectrum peculiarities, ³He abundance etc.) are especially discussed. Some unusual features of extreme solar events (e.g., 28 October 2003 and 20 January 2005) have been found in gamma-ray production and generation of relativistic particles (solar cosmic rays, or SCR). A number of different plausible assumptions are considered concerning the details of underlying physical processes during large flares: (1) existence of a steeper distribution of surrounding medium density as compared to a standard astrophysical model (HSRA) for the solar atmosphere; (2) enhanced content of the ³He isotope; (3) formation of magnetic trap with specific properties; (4) prevailing non-uniform (e.g., fan-like) velocity (angular) distributions of secondary neutrons, etc. It is emphasized that real progress in this field may be achieved only by combination of gamma-ray data in different energy ranges with multi-wave and energetic particle observations during the same event. We especially note several promising lines for the further studies: (1) resonant acceleration of the ³He ions in the corona; (2) timing of the flare evolution by gamma-ray fluxes in energy range above 90 MeV; (3) separation of gamma-ray fluxes from different sources at/near the Sun (e.g., different acceleration sources/episodes during the same flare, contribution of energetic particles accelerated by the CME-driven shocks etc.); (4) asymmetric magnetic geometry and new magnetic topology models of the near-limb flares; (5) modeling of self-consistent time scenario of the event.     

毛细芯蒸发器启动和运行特性

通过对毛细芯蒸发器(相当于环路热管在没有连接蒸气管路的情况)进行试验研究,巧妙地避开了工质循环和冷凝器等带来的影响,专注于研究毛细芯孔隙率和热源功率对蒸发器启动和运行特性的影响。结果表明:在某些条件下,毛细芯蒸发器启动时温度会出现剧烈的波动;毛细芯孔隙率越大,产生温度波动所对应的热源功率越小;毛细芯相同时,热源功率越大,越容易出现温度波动,并且温度波动的程度越剧烈。温度波动的原因是毛细芯孔隙率与热源功率等外部参数不匹配。     

基于FSS-kernelBSS方法的机械故障诊断

机械设备发生故障时,故障特征的提取是很重要的.为了从观测信号中分离出不同的故障特征源信号,并根据分离信号准确地进行故障诊断,从观测信号样本出发,提出了基于有限支持样本核函数的盲源分离(FSS-kernel BSS)方法.此方法利用有限的观测样本估计信号的概率分布,得到了评价函数,具有很好的自适应能力.仿真试验结果表明:此方法能成功地分离超、亚高斯混合信号,与其他盲源分离方法相比,此方法具有更好的分离性能.将该方法用于转子不平衡和支座松动的复合故障信号的盲分离,分离出了各复合故障的主要频谱.分离结果表明:此方法应用于机械设备复合故障诊断中是可行的.     

压扩与预失真结合的峰均功率比抑制方法

针对压扩法中峰均功率比抑制与系统误码率之间的矛盾,提出了一种压扩与预失真结合的方法.用Bussgang定理推导出正交频分复用信号经过非线性功率放大器后,在加性高斯白噪声信道下子载波信噪比的计算公式.用理想预失真代替非线性功放,再对线性压扩法进行改进.用理想预失真和改进后线性压扩的3个参数修改子载波信噪比计算公式,进而得到系统误码率.仿真结果表明:通过调整3个参数,在获得相同峰均比抑制效果及误码率的情况下,所提出方法的信噪比门限改善了0.8 dB.