复合材料构件热压罐成型温度场研究

在热压罐固化工艺的热历程中,复合材料零件表面温度场分布的合理与否将直接决定产品的固化质量.以工字型零件和T型加筋壁板两种复合材料零件为研究对象,使用EC-3×8M和SCH-5.5×21M两种型号热压罐,同时选择炉温偶和零件偶两种控温方式对零件进行固化.通过分析温度场测试结果发现,控温方式、设备加热方式、升降温速率、热电偶的摆放位置、固化压力等因素均对零件的温度场有影响.     

TC4钛合金静止轴肩和传统搅拌摩擦焊的温度场对比

基于有限元软件ABAQUS对6mm厚的TC4钛合金传统及静止轴肩搅拌摩擦焊温度场进行了有限元模拟.结果表明,对比传统搅拌摩擦焊接,静止轴肩搅拌摩擦焊接具有较小的高温区,前进方向上具有较大的温度梯度,厚度方向上呈现柱状椭球形分布,上、下表面温度峰值差异较小,具有重叠性较好的热循环曲线.     

RFID技术在航空领域的应用研究

射频识别(RFID)技术现已广泛用于物流、金融、零售等各个行业.航空领域的RFID应用起步较晚,通过对RFID技术在飞机制造商、原始设备生产厂家(OEM)、航空公司的一些典型的应用案例的分析,提出RFID技术应用于航空领域所面临的挑战及必要性,为其未来航空业自动识别技术的发展指明了方向.     

跨声速串列转子失速机制的数值研究

为了解决跨声速串列转子的低裕度问题,就必须了解跨声速串列转子的流场结构与失速机制.设计了叶尖切线速度为450m/s,负荷系数为0.56的高负荷跨声速串列转子.基于数值模拟的结果,分析了该串列转子在0.5mm叶尖间隙下的叶尖流场结构与失速机制,并在此基础上分别探讨了叶尖间隙和前、后排叶片周向位置对串列转子特性的影响和失速机制的变化.结果表明:前排叶片的叶尖区域是 影响串列转子稳定性的关键;随着叶尖间隙的增加,串列转子的失速机制也发生变化,从前排叶片叶尖区域的尾迹与径向潜流堵塞后排叶片通道转变为前排叶片叶尖泄漏流堵塞;在较大周向相对位置(后排叶片压力面周向远离前排吸力面)的情况下,串列转子获得最好的效果,随着周向相对位置(PP)的增加,失速部位从后排叶片转移至前排叶片.      

温度对飞机燃油射流泵工作特性影响

建立了射流泵数学模型,采用数值计算方法对其工作特性进行了模拟,搭建了实验台,采用RP-3燃油,通过实验数据验证了模型的正确性.在此基础上,分别选择了RP-3和JET-A两种燃油,计算了从-40℃~40℃温度下,不同操作压力对射流泵流量比的影响.结果表明:燃油温度高于0℃时,温度对射流泵工作特性影响并不明显,随着温度的降低,射流泵性能与标准温度下（20℃）偏差越来越大,且压比越高此偏差越明显.当温度高于0℃时,采用RP-3和JET-A燃油性能相差不大,RP-3燃油性能略优于JET-A燃油,但是在低温下,RP-3燃油性能远高于JET-A燃油.因此当燃油温度较低且压比较高时,必须充分考虑温度对射流泵特性的影响.      

导风轮叶片偏置对高压比串列离心压气机性能的影响

为提升高压比串列离心压气机的性能,借鉴常规一体化离心叶轮中偏置分流叶片的方法,针对某高压比串列离心压气机,应用数值仿真手段分析了串列叶轮中导风轮叶片周向偏置对压气机流场和性能的影响。通过对不同导风轮叶片偏置方案下压气机流场的分析,建立了压气机流动损失与偏置参数的关联性。研究表明:采用较大的偏置参数γ可降低导风轮叶片1前缘的激波强度,改善激波作用导致的泄漏涡破碎和流动分离,但过大或过小的γ方案中导风轮叶顶会出现二次泄漏致使低能流体的掺混损失增加;γ=65%方案压气机综合性能最佳,其压比和效率较γ=50%分别提高了1.5%和1.4%;对于串列离心压气机导风轮叶片周向位置的优化,在避免导风轮叶顶形成较强二次泄漏的前提下,应考虑采用较大的偏置参数γ,同时应防止诱导轮尾迹流体参与导风轮的叶顶泄漏。     

基于PIV技术的单圆孔脉冲射流流场特征

对稳态射流及脉冲射流冲击靶板时的流场特性结构进行了探索和分析。采用高频粒子图像测速技术,在射流管口到冲击靶板间距为6倍管径的条件下,对稳态射流进口雷诺数为6 000的稳态射流及脉冲频率为20 Hz的脉冲射流进行了实验测量,得到了射流核心区、壁面射流区及滞止区内的速度分布。研究发现:①由于射流剪切作用的影响,脉冲射流核心区的最大轴向脉动速度为稳态射流的3倍。②滞止区内,由于射流的剪切作用和壁面的滞止作用,导致了脉冲射流轴向速度梯度最大为稳态射流的2倍,同时,滞止区内的最大脉动速度是稳态射流脉动速度的3倍。③脉冲射流对壁面的卷吸以及旋涡的产生和传播过程,破坏了壁面射流区稳定的速度边界层。相比稳态射流,脉冲射流的流场增加了湍流相干结构的含能并产生周期性的大尺度卷吸涡。     

The effects of the solar magnetic polarity and the solar wind velocity on Bz-component of the interplanetary magnetic field

We have studied the effect of both solar magnetic polarity and the solar wind velocity on the Bz-component of the interplanetary magnetic field, IMFBz, for the minimum activity of the solar cycles 21, 22, 23 and 24. We made a statistical study of IMFBz in the first section which is considered as an extension of Lyatsky et al. (2003). They made a statistical study of IMFBz for two periods of minimum solar activity 22 and 23 related to 1985–1987 and 1995–1997 when the solar magnetic field had opposite polarity. Our results seem to be consistent with the results obtained by Lyatsky et al. (2003). We found that there is a dependence of IMFBz on the IMFBx and the solar magnetic polarity for the minimum periods of the selected four solar cycles. In addition, we found that there is a dependence of IMFBz on the solar wind velocity.     

Subsidence rate monitoring of Aghajari oil field based on Differential SAR Interferometry

Land subsidence, due to natural or anthropogenic processes, causes significant costs in both economic and structural aspects. That part of subsidence observed most is the result of human activities, which relates to underground exploitation. Since the gradual surface deformation is a consequence of hydrocarbon reservoirs extraction, the process of displacement monitoring is amongst the petroleum industry priorities. Nowadays, Differential SAR Interferometry, in which satellite images are utilized for elevation change detection and analysis – in a millimetre scale, has proved to be a more real-time and cost-effective technology in contrast to the traditional surveying method. In this study, surface displacements in Aghajari oil field, i.e. one of the most industrious Iranian hydrocarbon sites, are being examined using radar observations. As in a number of interferograms, the production wells inspection reveals that surface deformation signals develop likely due to extraction in a period of several months. In other words, different subsidence or uplift rates and deformation styles occur locally depending on the geological conditions and excavation rates in place.     

Solar flare forecasting model supported with artificial neural network techniques

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.