地面效应对火箭橇发动机尾喷管流场特性的影响研究

摘要：基于火箭撬地面试验的需要，设计了大载荷高加速的短轨火箭橇动力系统，并对地面效应对火箭发动机尾喷管流场的影响进行了理论和试验研究。文中采用FLUENT计算软件对不同条件下的火箭发动机尾喷管外流场进行了三维数值仿真，分析了单枚火箭以及双枚火箭工作时，地面效应对发动机尾喷管流场特性的影响。针对本文研究的大载荷高加速的短轨火箭撬动力系统，地面效应的影响和双尾喷管之间的相互作用都是在1.5ms时开始显现，在2ms~3ms时比较明显，在5ms~20ms开始减小，最后形成稳定的尾部流场。对于喷管出口直径275mm、轴线距离地面不小于472mm和双喷管轴线距离不小于680mm的火箭橇动力系统，在火箭橇运动起来20ms之后，地面效应影响和双火箭发动机之间相互作用变得非常小。     

空客A320鲨鳍小翼燃油节油性能分析

通过对比已选装和未选装鲨鳍小翼飞机的燃油消耗率,找出了节油效率和鲨鳍小翼改装成本之间的平衡点,为选装鲨鳍小翼的决策提供技术支持和数据参考。     

Experimental investigation on a cavity-step-actuated supersonic oscillating jet

Wind tunnel testing is conducted at different back pressures in a vacuum-type wind tun-nel for a novel supersonic fluidic oscillator which consists of a two-dimensional Laval nozzle, a rect-angular cavity and a backward step, to obtain its characteristics and the conditions for jet oscillating. The experimental results show that periodic asymmetrical flipping of the supersonic jet appears over certain nozzle pressure ratio (NPR) range according to schlieren visualization and pressure fluctuations. The jet flipping appears only when the jet is over expanded. The normal-ized average amplitude of the lateral pressure difference acting on the roofs of the cavity and the step varies around 0.2 while the periodic flipping appears. The supersonic jet periodic flipping fre-quencies obtained from the experiments agree well with those from the modified Rossiter mode for cavity-step acoustic resonance, but further investigations are needed to discover the underlying mechanism for the jet flipping.     

膜分离器及其机载应用

为了满足飞机放火防爆要求，膜分离器作为机载油箱惰化系统的关键部件在国外军、民机已经装机使用，在国内膜分离器处于研制阶段，正逐步向军、民用飞机推广应用。分析了国内外现状，对膜分离器工作机理进行了阐述，详细论述了膜分离器研制过程中涉及到的膜材料、膜制备工艺、膜分离器，总结了影响膜分离器性能的主要参数；进行了膜分离器在机载惰化中应用的试验研究，总结了研发和应用中得到的经验，有利于膜分离器今后的研发和机载惰化中的应用。     

浅析光学测量方法在修理企业零件制造方面的应用

介绍了应用光学测量方法还原无图零件、铸造件、磨损件以及测绘零件三维模型的方法，运用数控加工、增材制造等加工方法，实现了无图样零件的制造和检测。     

逆向喷流对双锥导弹外形减阻特性的影响

逆向喷流是一种主动流动控制技术，具有减阻降热特性，可用于高超声速飞行器设计。以典型双锥导弹外形的球头、单锥、双锥（全弹）为研究对象，将喷流发生器和弹体固连，采用CFD方法对逆向喷流的减阻特性进行了数值研究，对比分析了喷流马赫数、喷流压比等参数对不同对象减阻效果的影响。结果表明：逆向喷流流场存在长、短射流穿透两种模态；球头在小压比长射流模态时的减阻效果最佳；单锥和双锥在大压比短射流模态时的减阻效果更好。存在一个最佳压比，使得逆向喷流的减阻效果最佳；喷流压力过大，减阻效果变差，甚至出现阻力系数不降反增情形。逆向喷流减阻效果对控制体选取敏感，若将逆向喷流对头部的减阻特性（超过40%）直接推广至飞行器整机（6%左右），评估结果过于乐观。综合最佳减阻效果、最佳喷流压比、流量与所需储气瓶体积等影响因素，工程应用时逆向喷流应优先选用声速喷流。     

Thick exchange layer evaporation model with natural convection effect and evaporation experimental study for multicomponent droplet

In order to investigate the high-temperature evaporation characteristics of multicomponent liquid fuel, three kinds of blended fuel: n-heptane/n-decane/RP-3 aviation kerosene-ethanol were experimentally studied with and without forced convection. Further, based on zero-diffusion and infinite diffusion concept, this study expanded Thick Exchange Layer evaporation model with Natural Convection effect (NC-TEL) to multicomponent liquid fuels. The experimental results show that the droplet evaporation rate increases significantly with the increase of ambient temperature. Higher temperature leads to more significant relationships between the composition ratio and the evaporation rate. The effect of forced convection is not obviously under the circumstance in this paper. Then, the evaporation models were validated by experimental data. In general, the new NC-TEL model behaves better than the Ranz-Marshall (R-M) model, and the prediction accuracy at high temperature is improved by 8% to 35%. In lower temperature conditions, the prediction of zero-diffusion NC-TEL model is better than the infinite diffusion NC-TEL model. In high-temperature conditions, for n-heptane-ethanol droplet, the predictions of NC-TEL model are accurate, but for n-decane/RP-3 aviation kerosene-ethanol, the predictions are lower than experimental results. This may be caused by the micro-explosion phenomenon and the Marangoni phenomenon.     

基于EGView的SR20飞机的发动机爆震分析

基于EGView软件对SR20飞机出现的多起发动机CHT异常升高故障进行了分析，结果表明出现了早燃引发的爆震，进一步对爆震发生的几率以及如何减小爆震的强度和持续时间进行了研究，并就该机型在运行中减少爆震的发生提出了建议。     

Temporal evolution of the EIA along 95°E as obtained from GNSS TEC measurements and SAMI3 model

The total electron content (TEC) derived from GNSS measurements at a trans-hemispheric meridional chain of ground stations around 95°E longitude are used to study the quiet time inter-hemispheric structure and dynamics of the equatorial ionization anomaly (EIA) during the period March 2015 to February 2016. The stations are Dibrugarh (27.5°N, 95°E, 43° dip), Kohima (25.6°N, 94.1°E, 39° dip), Aizawl (23.7°N, 92.8°E, 36° dip), Port Blair (11.63°N, 92.71°E, 9° dip) and Cocos Islands (12.2°S, 96.8°E, 43° dip). The observation shows that the northern crest of the EIA lies in the south of 23°N (Aizawl) in all seasons but recedes further south towards the equator during December solstice. The largest poleward expansion of the northern (southern) EIA is observed in the March equinox (December solstice). The equinoctial and hemispherical asymmetry of TEC is noted. The winter anomaly is observed in the northern hemisphere but not in the southern hemisphere. The highest midday TEC over any station is observed in the March equinox. The TEC in southern summer (December solstice) is significantly higher than that in the northern summer (June solstice). The observed northern EIA contracts equatorward in the postsunset period of solstice but the southern EIA persists late into the midnight in the December solstice. The asymmetry may be attributed to the different geographic location of the magnetically conjugate stations. The SAMI3 simulations broadly capture the EIA structure and the inter-hemispheric asymmetry during solstices. The difference between observations and the SAMI3 is higher in March equinox and December solstice. The higher E?×?B vertical drift in the 90–100°E sector and the large geographic-geomagnetic offset in observing stations may have contributed to the observed differences.