焊接工艺对钛合金焊接接头冲击韧性的影响

介绍了俄罗斯对钛及其钛合金焊接接头冲击韧性最大值的影响因素的研究工作,以对相关航空研究作参考作用。     

Improvement of Baldwin-Lomax turbulence model for supersonic complex flows

Entropy represents the dissipation rate of energy. Through direct numerical simulation (DNS) of supersonic compression ramp flow, we find the value of entropy is monotonously decreasing along the wall-normal direction no matter in the attached or the separated region. Based on this feature, a new version of Baldwin-Lomax turbulence model (BL-entropy) is proposed in this paper. The supersonic compression ramp and cavity-ramp flows in which the original Baldwin-Lomax model fails to get convergent solutions are chosen to evaluate the performance of this model. Results from one-equation Spalart-Allmaras model (SA) and two-equation Wilcox k-x model are also included to compare with available experimental and DNS data. It is shown that BLentropy could conquer the essential deficiency of the original version by providing a more physically meaningful length scale in the complex flows. Moreover, this method is simple, computationally efficient and general, making it applicable to other models related with the supersonic boundary layer.     

MHD Spectroscopy of Transonic Flows

In previous publications (Keppens et al.: 2002, Astrophys. J. 569, L121; Goedbloed et al.: 2004a, Phys. Plasmas 11, 28), we have demonstrated that stationary rotation of magnetized plasma about a compact central object permits an enormous number of different MHD instabilities, with the well-known magneto-rotational instability (Velikhov, E. P.: 1959, Soviet Phys.–JETP Lett. 36, 995; Chandrasekhar, S.: 1960, Proc. Natl. Acad. Sci. U.S.A. 46, 253; Balbus, S. A. and Hawley, J. F.: 1991, Astrophys. J. 376, 214) as just one of them. We here concentrate on the new instabilities found that are driven by transonic transitions of the poloidal flow. A particularly promising class of instabilities, from the point of view of MHD turbulence in accretion disks, is the class of trans-slow Alfv’en continuum modes, that occur when the poloidal flow exceeds a critical value of the slow magnetosonic speed. When this happens, virtually every magnetic/flow surface of the disk becomes unstable with respect to highly localized modes of the continuous spectrum. The mode structures rotate, in turn, about the rotating disk. These structures lock and become explosively unstable when the mass of the central object is increased beyond a certain critical value. Their growth rates then become huge, of the order of the Alfv’en transit time. These instabilities appear to have all requisite properties to facilitate accretion flows across magnetic surfaces and jet formation.     

Stanvagon猜想的一个推广

本文推广了Stanvagon在文[1]中所提出的猜想。并给出了新的证明方法。     

High-order implicit discontinuous Galerkin schemes for unsteady compressible Navier–Stokes equations

Efficient solution techniques for high-order temporal and spatial discontinuous Galerkin(DG) discretizations of the unsteady Navier–Stokes equations are developed. A fourth-order implicit Runge–Kutta(IRK) scheme is applied for the time integration and a multigrid preconditioned GMRES solver is extended to solve the nonlinear system arising from each IRK stage. Several modifications to the implicit solver have been considered to achieve the efficiency enhancement and meantime to reduce the memory requirement. A variety of time-accurate viscous flow simulations are performed to assess the resulting high-order implicit DG methods. The designed order of accuracy for temporal discretization scheme is validate and the present implicit solver shows the superior performance by allowing quite large time step to be used in solving time-implicit systems. Numerical results are in good agreement with the published data and demonstrate the potential advantages of the high-order scheme in gaining both the high accuracy and the high efficiency.     

非均匀来流下三维激波反问题的微元密切轴对称解法

传统的密切轴对称理论被广泛应用于均匀来流下的三维密切曲面激波反设计，为解决非均匀来流条件下的三维曲面激波反问题，提出了一种微元密切轴对称流场（MOA）求解方法。该方法沿激波面的周向和流向构建一系列微元密切面，在每个微元面内进行三维向二维流动的等效转换，从而突破了传统密切方法中不能有横向波后流动的限制。利用该方法编写设计程序，分别基于带攻角来流条件和外锥型流来流条件重构了标准内锥曲面激波，并与数值仿真结果进行了比较。结果表明，非均匀来流下激波曲面的三维形状均与预设形状完全一致，实现了非均匀来流下曲面激波形状可控。MOA方法在吸气式高超声速推进领域中前体/进气道一体化设计方面有重要应用前景。     

飞机机翼表面霜冰的三维数值模拟

基于欧拉两相流理论对三维情况下飞机机翼表面的霜冰进行了数值模拟.根据水滴拟流体模型建立三维水滴控制方程;提出一套水滴控制方程的数值求解方法;由三维水滴流场的求解结果计算机翼表面的水滴收集特性,提出一种三维积冰外形的生成方法,完成了对飞机机翼表面霜冰的三维数值模拟.对ONERA M6机翼在不同迎角下霜冰的积冰情况进行了数值预测,并分析了结冰条件对积冰的影响.      

Numerical simulation of compression corner flows at Mach number 9

A hypersonic vehicle encounters a wide range of conditions during its complete flight regime. These flight conditions may vary from low to high Mach numbers with varying angles of attack. The near-wall viscous dissipation associated with flows at combined high Mach and Reynolds numbers leads to significant wall heat transfer rates and shear stresses. The shock wave/boundary-layer interaction results in a flow separation region, which commonly augments total pressure losses in the flow and lowers the efficiency of aerodynamic control surfaces such as fins installed on a vehicle. The standard turbulence models, when used to resolve such flows, result in incorrect separation bubble size for large separated flows. Therefore, it results in an inaccurate aerodynamic load, such as the wall pressures, skin friction distribution, and heat transfer rate. In previous studies, the application of the shock-unsteadiness correction to the standard two-equation k-ω turbulence model improved the separation bubble size leading to an accurate pressure prediction and shock definition with the assumption of constant Prandtl number. In the present work, the new shock-unsteadiness modification to the k-ω turbulence model is applied to the hypersonic compression corner flows. This new model with variable Prandtl number is based on the model parameter, which depends upon the local density ratio. The computed wall pressures, heat flux and flow field are compared to the experimental data. A parametric study is carried out by varying compression deflection angles, free stream Reynolds number and wall temperatures to compute the flow field and wall data accurately, particularly in the shock boundary layer interaction region. The new shock-unsteadiness modified k-ω model with variable Prandtl number shows an accurate prediction of initial pressure rise location, pressure distribution in the plateau region and heat flux in comparison to the standard k-ω model.     

时间矢量推进方法及其在叶轮机非定常流分析中的应用

为提高周期性非定常流动的求解效率,将非定常计算的初值问题转换为边值问题,提出了时间矢量推进方法,并将该方法应用于叶轮机多排的非定常流动分析中。通过对两排对转风扇进行非定常仿真,并对比双时间步计算方法的计算结果,讨论了新方法的计算效率,研究了该方法对排间干扰捕捉的准确性和可靠性。得到了以下结论:在物理时间步长相等的情况下,新方法与双时间步方法的计算结果基本一致,且计算时间约为双时间步方法的1/8;时间矢量推进方法能够很好捕捉排间的势扰动、熵扰动和涡扰动以及主流和扰动之间的非线性作用;时刻样本数较少会使时间矢量推进方法捕捉到的非定常变化幅值变小,且无法解析时间尺度较小的非定常流动现象。     

超高速高焓流动研究进展

本文介绍了中国科学院高温气体动力学重点实验室在超高速高焓流动模拟技术和试验方法方面取得的研究进展.文章主要包括三部分研究内容:第一部分是关于发展先进的超高速试验模拟技术,包括爆轰驱动高焓激波风洞和爆轰驱动高焓膨胀管.高焓激波风洞产生的超高速气流速度的范围是3.5km/s～6.0km/s,高焓膨胀管能够模拟速度为6.5km/s～10km/s的超高速气流.第二部分介绍高焓激波风洞喷管流场诊断结果,用来检验喷管产生的超高速流场的流场品质及其与飞行条件的差异.第三部分是关于超高速流动的试验方法和数值技术研究,包括高焓流动中真实气体效应对飞行器俯仰力矩变化的影响;热化学反应流动中表面催化效应诱导的气动热变化规律;喷管流场的气流非平衡效应对试验结果可能产生的影响.