离心风扇非定常气动力和气动噪声特性数值研究

将Lighthill方程转变为频域Helmholtz弱积分形式并采用Galerkin方法离散.基于声学有限元方法考虑声波在复杂固壁(叶轮和蜗壳)内的散射和反射等作用,利用Ffowcs Williams-Hawking(FW-H)方程耦合非定常流场计算结果数值预测了某离心风扇的噪声辐射,流场计算结果和蜗壳壁面动态压力测量结果在基频上吻合较好.结果表明:基频压力脉动分量在噪声源特性中占据主导地位且靠近叶轮前盖板对应位置的蜗舌区域(叶轮出口宽度范围内)是最主要的噪声源区域;声学有限元方法和实验吻合较好,复杂固壁对声传播影响不容忽略.叶轮出口不稳定气流对蜗壳周期性冲击引起的转/静干涉噪声远大于叶片偶极子源噪声是离心风扇最主要的噪声辐射分量且噪声主要从风扇管道出口方向传播.      

贫油预混预蒸发低污染燃烧室流场特性试验

采用粒子图像测速(PIV)技术测量带双环旋流多点燃油直接喷射(TAMI)头部的贫油预混预蒸发(LPP)低污染燃烧室流场特性,试验相同进口条件下冷态及喷雾燃烧时流场结构,通过分析平均流场涡量、湍流强度及切应变率等特性参数来详细说明喷雾燃烧对贫油预混预蒸发(LPP)低污染燃烧室流场的影响,并且研究了不同进口参数对其燃烧流场的影响.试验结果表明:①装有此头部的LPP低污染燃烧室喷雾燃烧流场回流区比冷态流场要小,并且平均流场特性参数在燃烧前后变化比较大;②随着进口油气比增加,中心回流区变短变胖;③随着进口空气量增加,回流区变窄变长.本试验所获得的流场特性结果可为低污染燃烧室的设计提供了一定的参考.      

超高速撞击声发射信号在Whipple结构中的传播时序特性研究

为研究屏/舱声发射信号传播时序特性,以典型Whipple防护结构为例,利用二级轻气炮对其进行超高速撞击实验。首先,利用独立于靶件的“遮挡板”阻挡弹丸击穿前板形成的二次碎片云撞击后板,利用布置在前、后板特定位置的超声换能器采集单纯的前板声发射信号,分析信号模态特征,结果表明：前板信号主要包括S0、A0和S2等三种模态板波,经圆柱支撑构件传播进入后板之后,全部转换为A0模态板波。在此基础上,建立了屏/舱声发射信号到达时序预测公式。其次,撤除遮挡板,利用布置在后板特定位置的超声换能器采集前、后板信号的混叠信号,分析两种信号的到达时序并与预测结果进行对比,结果验证了达时序预测公式的有效性。     

微型镓场发射电推力器的研制和点火特性

为了满足立方星等微纳航天器对推进系统的需求,研制出中国首台针式微型镓场发射电推力器。通过提高润湿温度解决了真空环境下镓难以充分润湿钨针等问题。实现了推力器的稳定点火,测试了不同润湿温度和不同几何参数下的点火特性。得到了发射电流随润湿温度提高、极间距减小和吸极内孔直径的增大而增大的关系。通过公式计算,给出了不同发射电流下的理论推力。通过电场仿真得到不同几何参数下的电场强度,揭示了几何参数影响发射电流的原因。     

直流式喷嘴开口率声学抑制能力影响

根据喷嘴长度和入口边界条件,将液体火箭发动机气液同轴式喷嘴简化为4类:四分之一波长闭管、二分之一波长闭管、四分之一波长开管和二分之一波长开管。采用线性声学理论对喷嘴入口开口率的声学抑制影响进行了研究,得到了入口开口率声学影响规律。结果表明:在标准长度和最佳长度2种条件下,开口率对喷嘴抑制能力的影响差别很大。合理选择开口率和喷嘴长度能够有效提高喷嘴抑制能力。研究结果可为喷嘴长度和入口射流条件优化设计、燃烧室声学振荡抑制提供参考。     

空间行波管阴极寿命试验研究

空间行波管是卫星通信系统中最重要的功率放大器,必须具有较长的工作寿命。空间行波管的寿命主要受阴极寿命的制约,因此为了保证空间行波管的长期在轨工作,需要开展大量的阴极寿命试验研究,并对阴极寿命进行预测。共投入50支电子枪进行寿命试验,累计进行寿命试验1823080h,最长单管寿命试验时间65411h。基于寿命过程中的逸出功变化,建立了空间行波管阴极寿命预测模型。预测空间行波管阴极在960℃_b（℃_b为亮度温度）支取1A/cm²发射电流密度时寿命超过43年;在980℃_b支取1A/cm²时寿命超过22年;在1000℃_b支取1A/cm²时寿命超过15年。预测结果表明,空间行波管阴极可以满足卫星通信系统应用的长寿命要求。     

Effects of dust polarity and nonextensive electrons on the dust-ion acoustic solitons and double layers in earth atmosphere

Propagation of dustion acoustic solitary waves (DIASWs) and double layers is discussed in earth atmosphere, using the Sagdeev potential method. The best model for distribution function of electrons in earth atmosphere is found by fitting available data on different distribution functions. The nonextensive function with parameter $q=0.58$ provides the best fit on observations. Thus we analyze the propagation of localized waves in an unmagnetized plasma containing nonextensive electrons, inertial ions, and negatively/positively charged stationary dust. It is found that both compressive and rarefactive solitons as well as double layers exist depending on the sign (and the value) of dust polarity. Characters of propagated waves are described using the presented model.     

On the origin of cosmic rays in the spiral galaxy NGC 3310

The problem of cosmic ray production in the spiral galaxy NGC 3310 is addressed by analysing and comparing optical and radio continuum data. Tentative results indicate that on global scales relativistic electrons may be produced in the shock front associated with teh density wave while on local scales extreme population I objects may be producing them. It is inferred that the same conclusions apply to all cosmic rays produced in the disk.     

Transfer element method with application to acoustic design of aeroengine nacelle

In the present survey, various methods for the acoustic design of aeroengine nacelle are first briefly introduced along with the comments on their advantages and disadvantages for practical application, and then detailed analysis and discussion focus on a kind of new method which is called ‘‘transfer element method'(TEM) with emphasis on its application in the following three problems: turbomachinery noise generations, sound transmission in ducts and radiation from the inlet and outlet of ducts, as well as the interaction between them. In the theoretical frame of the TEM, the solution of acoustic field in an infinite duct with stator sound source or liner is extended to that in a finite domain with all knows and unknowns on the interface plane, and the relevant acoustic field is solved by setting up matching equation. In addition, based on combining the TEM with the boundary element method(BEM) by establishing the pressure and its derivative continuum conditions on the inlet and outlet surface, the sound radiation from the inlet and outlet of ducts can also be investigated. Finally, the effects of various interactions between the sound source and acoustic treatment have been discussed in this survey. The numerical examples indicate that it is quite important to consider the effect of such interactions on sound attenuation during the acoustic design of aeroengine nacelle.     

波浪前缘静子叶片对高速轴流风扇单音噪声的影响

航空发动机压气机噪声与大型风洞压缩机噪声问题日益凸显,相关研究机构迫切需求新的降噪手段以指导大型叶轮机械降噪设计。为了探索波浪前缘静子叶片在大型叶轮机械降噪中的应用前景,采用非定常雷诺平均Navier-Stoke（URANS）方程与FW-H方程混合方法对基准静子叶片和3种波浪前缘静子叶片的降噪效果进行了数值模拟,研究对象静子来流平均马赫数约为0.49,基于静子叶片弦长的雷诺数约为1 040 000。数值预测结果显示：波浪前缘静子叶片可以显著降低高速轴流风扇单音噪声,但会对风扇的气动性能产生少许不利影响;相较于基准静子叶片,3种波浪前缘静子叶片可以在1BPF时降低风扇入口声功率级0.97~1.5 dB,2BPF时降低风扇入口声功率级2.89~4.9 dB,3BPF时降低风扇入口声功率级3.32~4.72 dB;同时,总压比降低0.1%~0.8%,等熵效率降低0.1%~0.3%。进一步研究表明：不同频率下声源振幅和相位关系是风扇单音噪声强度的主要影响因素,总的来说,幅值的增加会降低声源强度,然而通过改变声源相位关系的降噪方式则需要兼顾径向模态与波长两个方面。