CPL蒸发器多孔芯内传热传质的非稳态数值模拟

基于多孔芯内局部热力学平衡的假设，考虑了Brinkman和Forchheimer对Darcy定律的修正模型，针对简化的物理模型中所包含的气液相区域，建立了二维分层饱和多孔介质模型，以甲醇为工质对CPL，蒸发器毛细多孔芯内的传热传质过程进行非稳态数值模拟。在不同的热负荷条件下预测气液分层界面的形状和位置、系统由初态达到稳态过程的持续时间，讨论压力和温度的分布。由两层饱和模型所得到的计算结果可知．CPL系统在启动时，为避免高热流时液体脱离多孔区而发生干涸，宜采用小负荷启动；采用预热器，改善蒸气的出口条件；增加蒸发器入口处的工质的过冷度，有利于增加CPL系统启动过程和变工况时的稳定性。文中分析结论为CPL系统的优化设计提供参考。     

某型号液体火箭发动机可靠性分析

基于逐步增加Ⅱ型截尾样本,讨论了某型号液体火箭发动机可靠性指标的Bayes估计及E-Bayes估计.在刻度平方误差损失函数下,给出了火箭发动机寿命分布参数、可靠度函数及失效率函数的Bayes估计及E-Bayes估计.最后运用Monte Carlo方法对各种估计的均方误差进行了模拟比较.结果表明,E-Bayes估计给出的估计精度高.     

涡轮排气液化循环发动机的能量分析

对涡轮排气液化循环发动机液化水的处置进行了研究。通过热力学分析获得了发动机性能的理论解,并利用热力计算进行验证。分析表明液态水直接排出发动机将导致约2%的比冲损失。分析了发动机各环节的能量传递,获得了燃烧室中心燃烧区焓增的理论表达式,可作为燃烧室性能的详细分析的基础。     

锯齿尾缘叶片气动特性和绕流流场的数值研究

以基于NACA 0018翼型的锯齿尾缘仿生叶片为研究对象,采用大涡模拟的方法研究锯齿相对齿宽与相对齿高对锯齿尾缘叶片的气动特性和非定常绕流流场的影响规律和机制.研究表明,尾缘锯齿参数对叶片气动性能的影响是复杂的非线性过程,在一定来流攻角范围内能提高升阻比,但失速提前.如在9.4°~14.8°来流攻角范围内,不同相对齿宽系列叶片的升阻比高于原始叶片,升阻比与锯齿相对齿宽之间没有线性关系.研究还表明,锯齿尾缘能延迟边界层分离,加速尾迹的流动掺混和能量扩散,改变非定常涡结构和涡脱落频率.相对齿高的变化对非定常流动特性的影响更为显著.尾缘锯齿诱导的二次湍流射流和吸力面侧反向涡对改变了原始叶片的绕翼环量,进而影响锯齿尾缘叶片的气动特性和绕流流场特性.      

一种涡轮排气蜗壳的优化设计

为了改善涡轮排气蜗壳的排气效果,选取一种箱式蜗壳为原始计算模型,通过数值模拟研究了该排气蜗壳的气动性能,揭示了蜗壳内部流动损失的主要来源,在不改变其几何尺寸的前提下,提出了一种蜗壳的分流层改型设计,并与两种一般改型方式的效果作比较.数值计算结果表明:在设计工况下,分流层改型设计可使排气蜗壳的总压损失系数最多降低32.12%,静叶恢复系数最多提高48.73%,其效果好于扩压结构弧线改型,但弱于蜗壳壁面轮廓型线改型,在此基础上揭示了分流层设计改善蜗壳气动性能的机理.      

Coupled Lagrangian impingement spray model for doublet impinging injectors under liquid rocket engine operating conditions

To predict the effect of the liquid rocket engine combustion chamber conditions on the impingement spray, the conventional uncoupled spray model for impinging injectors is extended by considering the coupling of the jet impingement process and the ambient gas field. The new coupled model consists of the plain-orifice sub-model, the jet-jet impingement sub-model and the droplet collision sub-model. The parameters of the child droplet are determined with the jet-jet impingement sub-model using correlations about the liquid jet parameters and the chamber conditions.The overall model is benchmarked under various impingement angles, jet momentum and offcenter ratios. Agreement with the published experimental data validates the ability of the model to predict the key spray characteristics, such as the mass flux and mixture ratio distributions in quiescent air. Besides, impinging sprays under changing ambient pressure and non-uniform gas flow are investigated to explore the effect of liquid rocket engine chamber conditions. First, a transient impingement spray during engine start-up phase is simulated with prescribed pressure profile. The minimum average droplet diameter is achieved when the orifices work in cavitation state, and is about 30% smaller than the steady single phase state. Second, the effect of non-uniform gas flow produces off-center impingement and the rotated spray fan by 38°. The proposed model suggests more reasonable impingement spray characteristics than the uncoupled one and can be used as the first step in the complex simulation of coupling impingement spray and combustion in liquid rocket engines.     

基于HOG和SVM算法的磨粒图像在线监测技术

为了解决发动机润滑油液磨粒图像监测只适用于微流且易受气泡干扰等问题,设计了一种可适用于相对大流量工作环境的油液磨粒光学图像在线监测系统,区分气泡和磨粒。通过该监测系统,批量采集了一系列磨损颗粒和气泡图片,用于后续图像分类算法的训练与测试。采用了一种基于背景差分和大津法的运动物体提取算法提取出大量磨粒及气泡图像样本,运用基于方向梯度直方图（Histogram of oriented gradients,HOG）进行特征提取和支持向量机（Support vector machine,SVM）分类算法对气泡和磨粒进行识别。实验结果表明,该监测系统能有效采集磨粒及气泡图像并进行自动识别。与基于形态学特征提取算法以及K最近邻（K-nearest neighbor,KNN）等传统分类算法相比,HOG-SVM算法分类精度更高,识别准确率可达83 8%。     

A swept fin-induced flow field with different height mounting gaps

In order to apply the air fin successfully and ensure the maneuverability of hypersonic vehicle, a key problem to be studied urgently is the heat flux brought by the fin mounting gap. The appearance of mounting gap and fin shaft can induce many complex flow structures which need more attentions to be investigated. Under Ma 6, Nano-tracer-based Planar Laser Scattering (NPLS) and Temperature Sensitive Paints (TSP) were applied to visualize and measure transient flow structures and heat flux distribution of a swept fin-induced flow field with different height mounting gaps. Complementarily, Reynolds-averaged N-S equations were solved with k-ω SST turbulent model. The heat flux distribution results of numerical simulation and TSP observed the change of high heat flux region with different mounting gap, both in position and magnitude. The streamlines based on Computational Fluid Dynamics (CFD) and flow visualization results obtained by NPLS revealed the cause of high heat flux region. The high heat flux region in this flow field is mainly related to the reattachment of vortex and flow stagnation. The increase of gap height can lead to stronger gap overflow and shaft-induced horseshoe vortex, which are source of the high heat flux around the fin. The case with the highest mounting gap (4 mm) en-counters the most severe aerodynamic heating, both on the surface of fin and plate. Thus, under the premise of ensuring the flexibility of the fin, the gap should be set as small as possible.     

Case study of inclined sporadic E layers in the Earth’s ionosphere observed by CHAMP/GPS radio occultations: Coupling between the tilted plasma layers and internal waves

We have used the radio occultation (RO) satellite data CHAMP/GPS (Challenging Minisatellite Payload/Global Positioning System) for studying the ionosphere of the Earth. A method for deriving the parameters of ionospheric structures is based upon an analysis of the RO signal variations in the phase path and intensity. This method allows one to estimate the spatial displacement of a plasma layer with respect to the ray perigee, and to determine the layer inclination and height correction values. In this paper, we focus on the case study of inclined sporadic E (E_s) layers in the high-latitude ionosphere based on available CHAMP RO data. Assuming that the internal gravity waves (IGWs) with the phase-fronts parallel to the ionization layer surfaces are responsible for the tilt angles of sporadic plasma layers, we have developed a new technique for determining the parameters of IGWs linked with the inclined E_s structures. A small-scale internal wave may be modulating initially horizontal E_s layer in height and causing a direction of the plasma density gradient to be rotated and aligned with that of the wave propagation vector k. The results of determination of the intrinsic wave frequency and period, vertical and horizontal wavelengths, intrinsic vertical and horizontal phase speeds, and other characteristics of IGWs under study are presented and discussed.     

Diurnal and seasonal variations in long-term changes in the E-layer critical frequency

Long-term changes in the E-layer critical frequency, foE, at three stations of the European region (Juliusruh, Slough and Rome) and also at Moscow and Wakkanai stations are analyzed by the method developed by the authors and described in detail in the previous papers. It is found that Juliusruh and Slough stations demonstrate a well-pronounced change in foE (a trend) during two previous decades. At the same time, the same features of the behavior of the aforementioned trend k(foE) are obtained. The trend is positive and negative in the morning and evening hours, respectively. Similar diurnal behavior of k(foE) is found also for Moscow station but with lower absolute values of the trends. A well-pronounced seasonal behavior of k(foE) is detected at Juliusruh and Slough: the trend is minimal and maximal in the summer period and at the end of fall—beginning of winter, respectively. The maximal amplitude in the morning hours reaches +0.04?MHz per year, whereas the minimal amplitude in evening hours is ?0.06?MHz per year. No systematic changes exceeding by the magnitude 0.01?MHz per year are found for Rome and Wakkanai stations. It is assumed that the observed trends are related to changes (trends) in the meridional wind bringing NO molecules from the auroral oval to lower latitudes.