Baldwin-Lomax 模型在转静干涉流动中的应用

本文以拉格朗日方式研究叶轮机内动、静叶间的相互作用,通过直接跟踪流体涡团的时间历程,来描述流体的非定常流动过程。发展了代数湍流模型（Ｂａｌｄｗｉｎ－Ｌｏｍａｘ湍流模型）在尾迹中的应用方法,克服了其它数值方法中无法准确捕捉尾迹中心线的运动轨迹,以及计算出的边界层外的湍流涡粘性系数偏大的缺陷。用该方法对叶轮机内转子／静子相互作用过程进行了数值模拟,与实验的对照表明,该方法是可信的。数值结果还表明,采用该模型能正确地模拟出叶轮机内尾迹和各种旋涡等非定常因素的流动过程,从而为研究叶轮机内非定常流动及掺混过程提供了一个新途径。     

多功能数字控制陀螺仪表试验器控制系统的设计与实践

介绍一种采用数字控制技术的多功能陀螺仪表试验器控制系统的设计方法并提供了试验数据。实践表明该类试验设备具有转速范围宽、精度高、通用性好等特点,有良好的应用前景。     

预燃室三维湍流和燃烧过程的数值模拟 (Ⅰ)计算模型和方法

对液氧－煤油液体火箭发动机的预燃室进行三维维湍流流动与燃烧过程的数值模拟，流动采用圆柱坐标系中的三维N－S方程组，并用k-ε双方程测流模型闭合，用同位网格和SIMPLE算法求解，源项进行线性化处理以便于收敛；离散后的方程采用SIP法求解；燃烧采用单频快速不可逆化学反应，喷注单元和预燃室头部的喷雾可以考虑液滴颗轨道模型（PSIC），针对液氧－煤油液体火箭发动机的预燃室建立耦合计算软件，通过考核算例获得燃气流场，组合浓度场和温度场的合理分布。     

针对叶轮机流场分析的不同Spalart-Allmaras湍流模型评价

Spalart-Allmaras（SA）湍流模型在Reynolds-Average Navier-Stokes（RANS）方程求解中得到了广泛的应用。针对叶轮机数值模拟,国内外学者提出了很多修正的SA模型,但它们之间的对比少有研究。为此,综述了原始的SA（SA-standard）,SA-neg,SA-Helicity,SA-Ning及SA-R五种不同SA湍流模型。针对NASA Rotor 67和NASA Rotor 37,考察这五种湍流模型对数值计算稳定性的影响及对叶轮机内部流动细节捕捉的能力。研究表明：SA-standard和SA-neg湍流模型计算结果几乎相同;相比于SA-standard湍流模型,SA-Ning湍流模型计算的压比、效率和堵塞流量均较大;SA-R湍流模型模拟的激波/边界层干涉更严重,分离区域更大,计算的压比小,模型修正效果不理想;SA-Helicity湍流模型不仅能极大地提高计算的压比和流量范围,而且能提高计算的稳定性和失速工况下的计算准确性,但计算的堵塞流量和效率较小。     

氩气回路中微量水分的测量

在快中子反应堆的气体回路上,用露点仪测量了快堆几个覆盖气体系统氩气中杂质水分的含量.测量时,通过将露点仪的探头从干燥器中拔出,使露点仪的本底升高1～5μL/L后再进行测量,可以较快地得到测量结果,对于测量水分含量小于15μL/L的氩气,这是方便、可行的方法.     

雷诺数对涡轮叶尖流场影响的数值研究

采用基于压力修正的三维计算流体力学程序，结合雷诺应力湍流模型和剪切应力传输湍流模型加壁面函数的方法，对某一轴流涡轮转子叶尖间隙流场进行了数值计算研究，详细计算了不同涡轮叶尖间隙高度和来流湍流度条件下雷诺数对涡轮转子间隙流场的影响，最后计算了转子效率。结果表明：当泄漏流流经叶尖时因为叶尖剪切力做功有块总压增大区；雷诺数带来的影响比湍流度和叶尖间隙高度带来的影响要大，湍流度的变化对流场影响不大；雷诺数对泄漏涡尺寸的影响不大，但低雷诺数会引起流动分离，带来损失，当雷诺数在文中的范围内变化时，效率下降近八个百分点。     

表计库房智能化管理系统的探讨

采用现代信息技术、条形码管理技术、计算机网络技术和现代通讯技术的基于工作流的表计检定信息系统的解决方案,实现表计库房智能化管理。着重描述该系统的原理、工作流程及应用。     

Radio sounding of the solar wind acceleration region with spacecraft signals

Data from coronal radio-sounding experiments carried out on various interplanetary spacecraft are used to derive the empirical radial dependence of solar wind velocity and density at heliocentric distances from 3 to 60 solar radii for heliolatitudes below 60° and for low solar activity. The radial dependencies of solar wind power and acceleration are derived from these results. Summaries of the radial behavior of characteristic parameters of the solar wind turbulence (e.g., the spectral index and the inner and outer turbulence scales), as well as the fractional density fluctuation, are also presented. These radio-sounding results provide a benchmark for models of the solar wind in its acceleration region.     

Aerodynamic characteristics of unsymmetrical aerofoil at various turbulence intensities

A series of wind tunnel tests were performed to investigate the effect of turbulent inflows on the aerodynamic characteristics of the unsymmetrical airfoil at various turbulence intensities and Reynolds number. To assess the aerodynamic characteristics, surface pressure measurements were made over the unsymmetrical airfoil surface by using a simultaneous pressure scanner MPS4264 of Scanivalve make. Self-generated passive grids made of parallel arrays of round bars were placed at four different locations to generate various Turbulence Intensities (TI) in the wind tunnel. The location of the passive grid has been normalized in terms of considering the distance between the entry of the test section and the leading edge of the model. Based on the wind tunnel results, by comparing the baseline without grid low turbulence case TI = 0.51% with other turbulence generated cases like TI = 4.68%, 4.73%, 6.04% and 8.46% at different Reynolds number, it is found that the coefficient of lift increases with the increase in the turbulence intensity. Results also reveal that the flow featuring turbulence can effectively delay the stall characteristics of an airfoil by attaching the flow over the airfoil for an extended region. Additionally, attempts were made to understand the influence of turbulence on the aerodynamic hysteresis.     

翼型近尾迹流动的PIV研究—动力学机制

利用在线式互相关PIV(ParticleImageVelocimetry)系统,在低速风洞中对NACA0012翼型在雷诺数2.39×105,0°和4°攻角下的近尾迹流动进行了详细测量。实验结果表明,翼型近尾迹存在有序的涡街结构,涡街在尾缘处形成后,在向下游的迁移中,会经历一个发展壮大、失稳破碎的演化过程,流动从有序走向无序。翼型的近尾迹是一种以旋涡的运动学特性和动力学机制为主导的流动现象。本文着重探讨了翼型尾缘处的涡街形成机理,尾迹内的流动机制,以及近尾迹的流动稳定性。