基于LES方法的平板非定常激波/湍流边界层干扰研究

以高超声速发动机进气道湍流分离控制为应用背景,采用大涡模拟(LES)方法进行马赫数为3.0(唇口附近马赫数约为3.0)的激波/湍流边界层干扰(SWTBLI)流场机理研究.利用扰动循环引入的方法,先得到充分发展湍流场,然后根据斜激波关系式引入激波的方法进行激波/湍流干扰模拟.研究结果显示:充分发展湍流场在激波作用下产生逆...     

非线性EASM在激波与湍流边界层相互作用中的数值应用

采用基于k-ω湍流模型的非线性显式代数应力模型(EASM)对超燃冲压发动机常用的超声速凹槽、压缩拐角和侧壁压缩进气道简化模型的激波与湍流边界层的相互作用进行了计算,主要研究了EASM 模型对壁面压强、摩阻、Stanton数和壁面摩擦力线的计算精度,计算结果与SST(shear stress transport)模型进行...     

轴的扭转振动分析

用波方程描述轴的扭转振动，轴的振劝用空间与时间坐标来描述的，运动方程是偏微分方程。     

Dynamic processes in the outer heliosphere: voyager observations and models

We review recent Voyager 2 observations in the vicinity of 70 AU. The character of the solar wind plasma data between 2002 and 2003 changed to a regime in which the speed, density and magnetic field magnitude are positively correlated. The average speed of the solar wind at Voyager 2 increased between early 2003 and mid-2004, which we attribute to a return of fast coronal hole flow. We use solar wind data at Earth as input to numerical models which include the effect of pickup ions to model the radial evolution of the solar wind. The model reproduces the basic features of the observations. As a specific example, we investigate the propagation of the Halloween (Oct.–Nov.), 2003 storms in the outer heliosphere. The model predictions are in reasonable agreement with Voyager 2 observations.     

多层太阳大气模式中Alfven波的传播

将实际的太阳大气划分为多个等温层次，导出了均匀倾斜磁场下线性Alfven波通过任意多等温层的能量透射率，结果表明，两等温层模式与三等温层模式的结果存在本质的区别。在两等温层中，温度的跃变式增高对Alfven波起着高通滤波的作用，而三等温层中在高频端Alfven波的透射率显示为振荡形态，对实际大气温度模式的计算结果表明，太阳低层大气更适合于周期为数秒的Alfven波的能量传输。     

Martian obstacle and bow shock: origins of boundaries anisotropy

The origin of the anisotropy in the shape of the Martian obstacle and bow shock is analyzed using Mars Global Surveyor observations. The influence of MHD or ion pick-up effects on Martian obstacle position was to be small found, however, localized Martian crustal magnetization increases the thickness of the downstream planetary magnetotail by 500–1000 km in agreement with earlier Phobos 2 observations. A new analytical model is presented for Martian obstacle shape variation for different solar wind ram pressure. Elongation of the Martian BS cross-section in the direction perpendicular to IMF was confirmed while the shift of this cross section in the +Y direction of Martian interplanetary medium reference frame was discovered. The shift of BS cross section in the direction of interplanetary electric field was not revealed thus not conforming the idea that mass-loading play some role in BS control.     

高灵敏度莫尔偏折法及其在激波风洞流场中的应用

本文介绍了一种具有高灵敏度的莫尔偏折法，从理论上分析了其工作和测量原理。并把这种方法用于高超声速激波风洞中流场的显示和测量，获得了几种特殊模型流场的清晰莫尔偏折图，定量计算了高超声速激波风洞中带有凸起物模型三维密度场的分布。     

Cf / ZrB2 -SiC 复合材料的制备及抗热冲击性能

采用前驱体转化法制备Cf / ZrB2 -SiC 复合材料,对材料的热物理和热震性能进行了研究。采用 扫描电镜和X 射线衍射分析材料的微观结构及物相变化。结果表明:复合材料在1 700℃热震循环10 次材料 保持完整,表现出了良好的抗热震性能。通过微观结构分析,高温氧化后生成的多孔SiO2 氧化层能够吸收热 应力,缓解因热震带来的巨大温度差,ZrB2 组元的加入有效地提高了材料抗热震性。     

聚能爆破切割清理弹射通道技术

 考虑到飞机隐身等因素,飞机驾驶舱顶部为金属结构而不是传统的座舱盖结构,在弹射救生过程中,采用聚能爆破切割技术,切割金属结构形成"座舱盖"并抛放以清理弹射通道,且已在B-1B、B2飞机上采用。利用座舱顶部金属结构平板件,对聚能切割器装药量、切割厚度,切割过程冲击噪声对飞行员的影响、爆破飞溅物对飞行员的损伤防护等进行了分析和试验研究,并将冲击噪声对飞行员的影响与国军标的要求进行了对比。通过本次研究,将为以后的工程应用提供基础性依据。     

Subsonic impulsively starting flow at a high angle of attack with shock wave and vortex interaction

Impulsively starting flow, by a sudden attainment of a large angle of attack, has been well studied for incompressible and supersonic flows, but less studied for subsonic flow. Recently, a preliminary numerical study for subsonic starting flow at a high angle of attack displays an advance of stall around a Mach number of 0.5, when compared to other Mach numbers. To see what happens in this special case, we conduct here in this paper a further study for this case, to display and analyze the full flow structures. We find that for a Mach number around 0.5, a local supersonic flow region repeatedly splits and merges, and a pair of left-going and right-going unsteady shock waves are embedded inside the leading edge vortex once it is sufficiently grown up and detached from the leading edge. The flow evolution during the formation of shock waves is displayed in detail. The reason for the formation of these shock waves is explained here using the Laval nozzle flow theory. The existence of this shock pair inside the vortex, for a Mach number only close to 0.5, may help the growing of the trailing edge vortex responsible for the advance of stall observed previously.