燃料分级对旋流火焰的动态特性影响研究

为深入研究分级旋流火焰特性,以分级旋流模型燃烧室为研究对象,对四个不同燃料分级比(Rf)条件下的分级旋流火焰进行了数值研究,在时均燃烧场特性分析的基础上进一步对燃料分级比为1和3两个工况进行了基于壁面建模的大涡模拟(WMLES)研究。结果表明:燃料分级比的改变会影响中心回流区(CRZ)的长度和宽度。燃烧室中截面的散点分布图能够显示出不同燃料分级比条件下的燃烧特征。燃料分级比为1时,燃烧室剪切层仅存在零散的涡破碎区;而燃料分级比为3时,伴随涡破碎区还出现了单螺旋分支进动涡核(PVC)。通过FFT变换获得的燃烧室内剪切层速度能谱主频与进动涡核的旋转频率相同,表明内剪切层速度脉动的产生与进动涡核有关。另外进动涡核会使流场内的燃料分布和燃烧模式发生周期性的变化,进而影响燃烧过程。调整燃料分级比在1附近,能够使分级火焰达到稳定燃烧降低排放的目标。     

介质阻挡放电等离子体的温度测量

在空气介质阻挡放电中,利用氮分子振动谱线和氮分子离子的转动谱线,研究了振动温度和转动温度在两极板间的分布情况。结果表明：越靠近极板振动温度越小,中间振动温度最高;而转动温度在两极板间基本保持不变。     

运输环境中某战术导弹结构振动特性分析

应用三维有限单元和导弹实体简化模型对一种战术导弹的结构振动特性进行分析，并动用ＡＮＳＹＳ有限元分析程序，计算得到了“自由－固支”条件下，导弹竖立状态的固有模态，取得了与试验和数据基本一致的结果，证明了所建模型物正确性，进而对运输环境中导弹水平支承条件下的固有频率和振型进行了分析计算，所得结果为导弹的使用可靠性分析提供了依据。     

基于特征空间变换的运载火箭Pogo模型降阶方法

针对运载火箭Pogo状态空间模型存在维数高和奇异性的问题,开展了Pogo模型的降阶方法研究。基于特征空间变换理论,导出了一般形式的Pogo状态空间模型的解耦形式。该形式与推进系统和结构系统的模态频率相对应,从而通过模态截断或保留感兴趣的模态实现有效的模型降阶。同时,还给出了降阶方法的实数运算公式。在两种不同型号推进系统的火箭Pogo问题中进行了仿真校验。结果表明所提出的降阶方法对奇异和非奇异Pogo状态空间模型都能给出正确的降阶模型,显著地提高计算效率,具有很好的通用性,为Pogo时域仿真和主动抑制提供了合适的模型。     

Gray bootstrap method for estimating frequency-varying random vibration signals with small samples

During environment testing, the estimation of random vibration signals （RVS） is an important technique for the airborne platform safety and reliability. However, the available meth- ods including extreme value envelope method （EVEM）, statistical tolerances method （STM） and improved statistical tolerance method （ISTM） require large samples and typical probability distri- bution. Moreover, the frequency-varying characteristic of RVS is usually not taken into account. Gray bootstrap method （GBM） is proposed to solve the problem of estimating frequency-varying RVS with small samples. Firstly, the estimated indexes are obtained including the estimated inter- val, the estimated uncertainty, the estimated value, the estimated error and estimated reliability. In addition, GBM is applied to estimating the single flight testing of certain aircraft. At last, in order to evaluate the estimated performance, GBM is compared with bootstrap method （BM） and gray method （GM） in testing analysis. The result shows that GBM has superiority for estimating dynamic signals with small samples and estimated reliability is proved to be 100% at the given confidence level.     

基于转子初始不平衡量控制的整机振动排故方法

针对某型航空发动机试车低压振动超限问题,结合发动机的结构特点,进行了故障分析。通过改进转子的平衡工艺,提出了控制转子初始不平衡量从而抑制发动机临界转速振动大的排故方法,再次试车时发现振动水平良好。结果表明排故方法有效,对今后发动机装配和整机振动排故具有重要的参考价值。     

基于主动失谐优化的叶轮瞬态加减速振动抑制

提出了一种基于主动失谐优化的叶轮瞬态加减速振动抑制方法.首先建立了瞬态加减速激励下的叶轮降阶模型,获得了表征失谐对瞬态振幅影响的失谐放大因子.然后基于降阶模型,采用蒙特卡洛仿真快速计算了一系列瞬态激励下失谐放大因子的概率密度分布,结果表明:失谐放大因子在大多数瞬态激励下受到随机小失谐的影响大于在稳态激励下受到的影响,且...     

Gamma ray astrophysics and signatures of axion-like particles

We propose that axion-like particles (ALPs) with a two-photon vertex, consistent with all astrophysical and laboratory bounds, may lead to effects in the spectra of high-energy gamma-ray sources detectable by satellite or ground-based telescopes. We discuss two kinds of signatures: (i) a peculiar spectral depletion due to gamma rays being converted into ALPs in the magnetic fields of efficient astrophysical accelerators according to the “Hillas criterion”, such as jets of active galactic nuclei or hot spots of radio galaxies; (ii) an appearance of otherwise invisible sources in the GeV or TeV sky due to back-conversion of an ALP flux (associated with gamma-ray emitters suffering some attenuation) in the magnetic field of the Milky Way. These two mechanisms might also provide an exotic way to avoid the exponential cutoff of very high energy gamma-rays expected due to the pair production onto the extragalactic background light.     

一种用于ACSR的主从机并行处理系统

以微机、ＬＨ－ＳＣ１６Ａ型Ａ／Ｄ板、ＳＣ５０型Ｄ／Ａ板以及ＴＭＳ３２０Ｃ３０Ａ型ＤＳＰ板为基础，建立了时域结构响应主动控制的主从机并行处理系统。这一系统具有多通道快速运算能力，可提高控制系统的控制律，更新速率，改善控制系统的跟踪能力。     

X-Ray Emission from Flare Collapsing Trap

An acceleration process in the collapsing magnetic trap, formed in the flare with cusp magnetic field topology, is described. Computations show that high-energy electrons are accumulated in the central part of the collapsing magnetic trap due to an increase of their pitch angles. The effect explains in a natural way the formation of X-ray loop-top sources. Then, using the model with the collapsing trap and considering only the adiabatic heating process, a possible explanation for the motion of the X-ray loop-top source observed at the beginning of some cusp-type flares is presented.