Numerical investigation of of nozzle cavities thermal radiation characteristics with center cone cooled

航空发动机高温部件是发动机3-5μm上的重要红外辐射之一,对高温部件之一的中心锥的红外抑制技术进行了数值研究．在中心锥前端布置气膜缝槽,缝槽几何参数经过优化设计,将部分外涵低温气流经过支板引入中心锥,对支板和锥体壁面形成冲击冷却,在锥体前端形成气膜覆盖,使得支板与中心锥壁面得到了有效冷却,两者平均温度分别降低21．1％和46．2％,冷却气量约为外涵流量的1．6％．喷管腔体3～5Izm波段上红外辐射得到有效抑制,喷管正后方红外辐射相比原型喷管降低30％,0°-45。范围内红外辐射则明显降低．     

叶片全三维反问题优化设计方法

基于数值求解Navier-Stokes方程,对叶轮机械叶片全三维反问题优化设计方法进行研究.反问题给定叶片表面的静压分布反求叶型,假设叶表网格点有虚拟移动速度,迭代过程中根据叶表的实际静压和目标静压之差来修改叶型.对单排叶栅进行了反问题设计,并给出了初步的优化算例,结果能很好地满足目标静压分布,验证了该方法的有效性,计算的时间和精度也适合进行工程应用.      

立楔诱导高超声速分离流动的被动控制研究

双模态超燃冲压发动机由于压力扰动可能发生不起动现象,造成推力严重下降,对飞行稳定性与飞行安全具有很强的破坏性.不起动初始阶段主要受到激波与边界层相互作用引起的流动分离影响,希望通过控制分离达到改善流动的目的.采用5阶特征型WENO(weighted essentially non-oscillator)格式与3阶TVD(total variation diminishing)型Runge-Kutta(R-K)格式的高精度数值方法,求解三维Navier-Stokes(N-S)方程,研究与分析了凸起物和被动吹吸两种被动控制方法对激波与边界层相互作用导致的高超声速流动分离现象的控制效果.结果表明:凸起物通过诱导流向涡形成,改变空间压力分布,减弱二次分离,影响分离结构;吹吸方式的被动控制技术通过平衡分离区与再附区之间的高低压差,降低逆压梯度,使压力分布与分离区域发生改变.      

激光冲击强化提高主动连杆振动疲劳性能

针对某型发动机放气活门主动连杆转接R处的疲劳断裂问题,进行了主动连杆激光冲击强化工艺研究;完成了原型件和激光冲击强化、喷丸及加大R3种处理工艺后主动连杆振动疲劳对比试验.结果表明,在317MPa的应力水平下,激光冲击强化、喷丸和加大R后主动连杆疲劳寿命分别为原型件的5.24倍、3.89倍及1.36倍;与其它2种工艺相比,激光冲击强化具有强化效果好、工艺稳定性高、易于实现等优点,是截至目前减少主动连杆疲劳断裂故障的最佳处理工艺.主动连杆激光冲击强化后表面粗糙度较小,产生深度约1.4mm的高数值残余压应力层,表层晶粒细化至纳米晶并伴随高密度位错.三者共同作用可以有效缓解转接R处的应力集中,抑制疲劳裂纹在转接R处的萌生和扩展,是主动连杆振动疲劳寿命提高的主要原因.     

射流对高超声速进气道起动性能的影响

为探索利用射流技术降低进气道起动马赫数的可行性,对二元高超声速进气道二维流场进行了数值模拟,通过对比不同工况的流场结构、流量系数及总压恢复系数,分析了射流对高超声速进气道的作用效果,并研究了射流速度、压强及倾角对进气道起动性能的影响。分析结果表明:施加射流,激波与进气道边界层原有干扰形式发生改变,是降低进气道起动马赫数的主要原因。研究还表明,增大射流速度利于提高控制效果,但持续增大射流速度,会造成隔离段反压升高,并且这一现象与射流压强相关,降低射流压强能使进气道起动的射流速度区间扩大,同时在不同射流倾角下,上述规律表现一致。该研究揭示了进气道起动能力随射流参数变化的系统性规律,可用于指导工程设计及优化。     

The heliospheric modulation of cosmic rays: Effects of a latitude dependent solar wind termination shock

Observations made with the two Voyager spacecraft confirmed that the solar wind decelerates to form the heliospheric termination shock and that it has begun its merger with the local interstellar medium. The compression ratio of this shock affects galactic cosmic rays when they enter the heliosphere. Hydrodynamic (HD) models show that the compression ratio can have a significant latitude dependence; with the largest value in the nose direction of the heliosphere, becoming significantly less towards the polar regions. The modulation effects of such large latitude dependence are studied, using a well-established numerical drift and shock modulation model. We focus on computing the modulated spectra for galactic protons with emphasis on the radial and polar gradients in the equatorial plane and at a polar angle of θ = 55°, corresponding to the heliolatitude of Voyager 1. Two sets of solutions are computed and compared each time; with and without a latitude dependence for the compression ratio. All computations are done for the two magnetic field polarity cycles assuming solar minimum conditions. Including the termination shock in the model allows the study of the re-acceleration of galactic protons in the outer heliosphere. We find that for the A < 0 polarity cycle the intensity between ∼200 MeV and ∼1 GeV in the vicinity of the shock in the heliospheric equatorial plane may exceed the local interstellar value specified at the heliopause. Unfortunately, at θ = 55°, the effect is reduced. This seems not possible during an A > 0 cycle because significant modulation is then predicted between the heliopause and the termination shock, depending on how strong global gradient and curvature drifts are in the heliosheath. The overall effect of the shock on galactic protons in the equatorial plane is to reduce the total modulation as a function of radial distance with respect to the interstellar spectrum. Making the compression ratio latitude dependent enhances these effects at energies E < 200 MeV in the equatorial plane. At larger heliolatitudes these effects are even more significant. The differences in the modulation between the two drift cycles are compelling when the compression ratio is made latitude dependent but at Earth this effect is insignificant. A general result is that the computed radial gradient changes for galactic protons at and close to the TS and that these changes are polarity dependent. In line with previous work, large polarity dependent effects are predicted for the inner heliosphere and also close to the shock’s position in the equatorial plane. In contrast, at θ = 55°, the largest polarity effect occurs in the middle heliosphere (50 AU), enhanced by the latitude dependence of the compression ratio. At this latitude, the amount of proton modulation between the heliopause and the termination shock is much reduced. If galactic cosmic rays were to experience some diffusive shock acceleration over the 100–1000 MeV range at the shock, the radial gradient should change its sign in the vicinity of the shock, how large, depends on the compression ratio and the amount of drifts taking place in the outer heliosphere. The effective polar gradient shows a strong polarity dependence at Earth but this dissipates at θ = 55°, especially with increasing radial distance. This tendency is enhanced by making the compression ratio latitude dependent.     

拦截器点火冲击模拟试验技术研究

介绍了拦载器的点火冲击地面模拟技术研究。通过梯形波冲击和波形复现试验模拟,测量出了导引头和惯组的角速率差别,并通过控制轨控力的方式获得了角速率频响函数,为结构修改和制导控制系统改进提供了重要依据。     

碳酚醛-铝板中二维X射线热击波数值模拟

文章利用平面应变正交各向异性材料率相关性的弹塑性本构模型和各向同性材料理想弹塑性本构模型,采用有限元方法编写程序,对X射线辐照碳酚醛-铝板时诱导的热击波进行数值模拟,讨论了热击波的传播规律。结果表明,在1 keV的 X射线辐照下,X射线穿透极浅,材料表面发生气化现象,应力峰值较大;在3 keV的X射线辐照下,X射线穿透较深,热击波呈现双波结构,材料的层裂更明显。     

月球着陆器着陆缓冲性能研究

首先基于MSC.Nastran/MSC.Adams软件建立了模拟月球着陆器的动力学模型,并利用模拟月球着陆器在地面冲击试验来验证仿真模型的正确性,重点关注缓冲机构与结构连接处的载荷,结构特征点的加速度响应,以及缓冲器的工作行程。然后利用模拟着陆器地面试验结果修正动力学分析模型,研究表明：着陆器结构和缓冲机构的柔性对缓冲性能具有较大的影响。最后,把动力学分析模型中的模拟结构更换成真实结构,进行着陆器在月球表面的着陆冲击仿真分析,从而获得模拟着陆器地面试验与着陆器在月面着陆的冲击缓冲性能差异。     

旋转对冲击射流流动及换热影响的数值研究

为了探究旋转对动叶前缘冲击射流流动及换热的影响机制,采用数值模拟的方法对比分析了静止条件和三种不同旋转转速下的流场结构与换热情况。结果表明:冲击靶面的平均努塞尔数随转速的增大而减小,最高转速下,靶面平均努塞尔数下降约16%。另一方面,压力面和吸力面侧对旋转的敏感性不同。高转速下,换热的削弱主要集中在吸力面和压力面无量纲弧长s/d小于2的区域,压力面s/d大于2区域的换热略有增强;旋转对流场结构产生了明显的影响,旋转改变了射流孔的流量分配,在科氏力的作用下,射流向压力面偏转,这种特征随转速的增大而更加显著。另外,旋转通道内的离心力改变了局部横向流强度。