采用二维贝叶斯方法求解旋转盘腔导热反问题

为了研究压气机旋转盘腔换热特性,实现准确求解转盘表面传热系数,引入二维贝叶斯方法,此方法采用先验分布优化测温误差,并且更加符合转盘的二维特性。通过加入噪声的模拟数据验证方法的可行性,结果表明无测温误差时方法的平均误差是3.2%,有测温误差时方法的平均误差是10.6%,并分析了误差来源。通过与已有实验结果对比,发现方法更适用于计算转盘迎风面与背风面传热差异较大时的表面传热系数,平均相对误差为9.6%,满足实际工程精度的要求。通过改变盘面温度测点数量,发现测点增加会提升计算精度,并采用统计抽样理论分析原因,发现在可接受误差为10%时,所需要的测点数量比较合理。     

MPT方法中的纳米粒子识别技术

多粒子追踪（MPT）是测量粒子布朗运动的一种方法。在200nm粒子扩散系数实验测量中,对MPT方法中的粒子识别和粒子匹配两个重要环节提出改进：在粒子识别时,通过调节灰度阈值并检测光斑面积的改变,可有效分别真实粒子和光晕引起的＂伪粒子＂;在粒子匹配中,将手动追踪和程序追踪得到的粒子单步位移用矢量法表示,可直观显示不同追踪方法的粒子匹配效果。实验结果表明,在MPT方法中增加上述措施后,手动追踪和程序追踪获得的实验扩散系数之间的偏差由8%~13%减小为2%~8%,说明基于阈值敏感性的＂伪粒子＂剔除方法合理、有效。     

旋翼翼型高速风洞试验壁压法修正研究

基于已有的单参数线化壁压信息法,在做相应简化改动后应用于旋翼翼型高速试验数据修正,着力解决工程上遇到的旋翼翼型高速风洞试验结果不理想的问题。文中采用该方法对FL-21风洞得到的OA309旋翼翼型试验数据进行了修正。结果表明,修正后的旋翼翼型气动特性曲线与国外已有结果吻合较好。该方法能有效满足旋翼翼型高速风洞试验修正的需要。     

基于有效透气量对火星降落伞气动力系数预测分析

针对火星探测任务中降落伞开伞环境为低密度大气的特点,本文由降落伞气动力系数与透气量关系,提出了通过降落伞有效透气量预测降落伞气动力系数的方法,该方法先由织物透气量试验获取伞衣透气量拟合曲线和透气量常数,再根据风洞试验得到两种有效透气量下的气动力系数,然后由有效透气量插值获取了盘缝带(DGB)伞火星大气条件下气动力系数,并且通过空投试验数据对该方法进行验证。计算结果表明,在火星条件下,降落伞气动力系数与风洞条件下变化趋势基本一致。Ma 0.4工况阻力系数的变化范围为0.583～0.622,Ma 0.8工况阻力系数的变化范围为0.438～0.494。     

Aeroacoustic and aerodynamic optimization of propeller blades

It is of great significance to develop a high-efficiency and low-noise propeller optimization method for new-generation propeller aircraft design. Coupled with free form deformation method, dynamic mesh interpolation technology, optimization algorithm, surrogate model, aerodynamic calculation and aeroacoustic prediction model module, the integrated aerodynamic and aeroacoustic design method of propeller is built. The optimization design for the six-blade propeller is carried out. The non-reduction in efficiency, thrust coefficient and the minimum of aerodynamic noise is treated as the optimization design objective. The spatial vorticity distribution of the propeller before and after the design is also analyzed by using unsteady computational fluid dynamics method. The results show that the optimized propeller can effectively reduce the aerodynamic noise level. The maximum total sound pressure level can be reduced by 5 dB without reducing its aerodynamic performance. The developed method has good application potential in low-noise optimization design of propeller and other rotating machinery.     

正弦波型高频动态压力光学校准系统及其应用

动态压力是气动部件表面的关键气动参数。光学压力敏感涂料（PSP）测量技术在测量气动部件表面动态压力方面具有全域测量、不影响流场自身的优势，而光学压力敏感涂料的动态响应特性则是进行动态压力测量的决定性因素。基于声学驻波管原理，自主设计并组建了正弦波型高频动态压力光学校准系统，主要包含有驻波管型校准舱、声源、激光源、高频压力传感器、光电倍增管以及测控系统。对动态压力光学校准系统及某新型快响压敏涂料的实验结果表明，所组建的动态压力校准系统可产生最短响应时间12.5 μs、最大压力幅值为4.37 kPa的正弦型动态压力，其有效动态频响范围为0.4~20.0 kHz（50 μs~2.5 ms），不确定度小于0.004 9%；校准系统合理的光路布局可进行快响压敏涂料动态特性的校准，所测涂料可用于动态频响不高于9.1 kHz（响应时间为109.9 μs）的非定常流场的压力测量。     

Temporal evolution analysis of storm-enhanced density during an intense magnetic storm on March 2015

An intense Storm Enhancement Density (SED) event with the magnetic storm occurred on 17–24 March 2015 has been investigated. The morphological character of the SED during different phase of the magnetic storm is examined and compared with the non-storm time. Three intensity indexes, i.e., “general” SED index, “heavy” SED index and “severe” SED index, are defined to represent the intensity of SED respectively represented by the numbers of the ionospheric total electron content (TEC) grids with TEC > 60 TECu, TEC > 80 TECu and TEC > 100 TECu. The temporal evolution of the SED intensity indexes during a time span covering the non-storm time and the magnetic storm time have also been investigated. The SED exhibits a shape with two parallel slender troughs in the middle and low latitudes during the non-storm time and then gradually develops into an ellipse structure as the development of magnetic storm. The intensity of SED and the fluctuation of the TEC evolution are generally corresponding to the fluctuation of Dst index. The analyzing results enrich our understanding of the temporal and spatial evolution of the ionospheric SED.     

On the detection of anomalous seismo-ionospheric behavior in the presence of space weather stimuli for large earthquakes

Anomalous behavior of ionospheric total electron content (TEC) prior to earthquake has been observed in many studies. Evidence of such seismo-ionospheric coupling effects suggests that it is plausible to rely on TEC signatures for early earthquake warning. However, the detection of pre-earthquake TEC anomalies (PETA) has not been adopted in practice due to two pertinent issues. Firstly, the effects of space weather activity can affect TEC levels and cause anomalous behavior in the TEC. Usually arbitrary thresholds are set for space weather indices to eliminate TEC anomaly due to space weather effects. Secondly, the choice regarding moving time-window length used to characterise background variation of TEC within the statistical envelope approach has an effect on detection of PETA. While the rule-of-thumb in selecting the moving window length is to have a time window capable of capturing background variability and short-term fluctuations, the length of the time window used in the literature varies with little justification. In this study, a critical examination is conducted on the statistical envelope approach and in particular, to eliminate the effect of space weather activity without the use of arbitrary space indices to detect PETA. A two-part PETA identification procedure is proposed, consisting of wavelet analyses isolating non-earthquake TEC contributions, followed by the statistical envelope method using a moving window length standardized based on observed periodicities and statistical implications is suggested. The approach is tested on a database of 30 large earthquakes (M?≥?7.0). The proposed procedure shows that PETA can be detected prior to earthquakes at higher confidence levels without the need to separately check for space weather activity. More importantly, the procedure was able to detect PETA for studies where it was previously reported that PETA could not be detected or detected convincingly.     

泡状隔板对涡轮叶片内冷通道换热和流阻的影响

为增强涡轮叶片内部通道的换热、减小流动阻力,提出了一种新型的泡状隔板结构。通过实验与数值模拟相结合的方法,研究了等热流边界条件下泡状隔板结构的半径以及形状对通道换热和流阻特性的影响,并与直隔板进行对比,实验结果表明:在研究范围内,对称型泡状隔板结构能够大大减小通道流动阻力,随着泡状结构半径的增大,减阻效果增强;不对称型泡状隔板结构只在半径最大时能减小流动阻力;泡状结构对于换热的影响并不明显。实验结论可以为涡轮叶片内部冷却通道的优化设计提供理论依据。     

压力波对垂直管低温气液掺混冷凝的影响

为了分析高压补燃液氧煤油发动机氧泵间管内气液两相掺混冷凝及其压力波传播过程,建立了可产生压力扰动的垂直管低温气液两相掺混实验系统,以氧气/液氧为实验工质,开展压力波对垂直管内低温气液两相掺混冷凝的影响研究,获得了不同压力波频率和氧气流量工况下的掺混图像,分析结果表明:压力波会使发散流型由微弱振荡冷凝向间歇振荡冷凝转变,使椭圆流型由稳定冷凝向振荡冷凝转变;在0~52 Hz不同频率压力波作用下,发散流型最大轴向冷凝长度与掺混孔径之比在10~30之间,椭圆流型的比值在8~15之间变化;压力波对气相摆动频率起主导性和正相关性的影响。