II型裂纹扩展与绝热剪切带传播的数值对比

通过数值计算的方法,对比绝热剪切带内裂纹扩展和预制II型疲劳裂纹扩展的动态性能参数。分析热塑失稳现象中裂纹的传播与绝热剪切带传播的关系。采用ABAQUS/CAE进行二维模型建立,预制疲劳裂纹和绝热剪切带,分析计算了材料在2种情况的应力应变时间曲线、II型动态应力强度时间历程以及裂纹扩展速度。计算结果表明,预制绝热剪切带与预制疲劳裂纹对于材料的破坏方式影响一致,即裂纹跟随绝热剪切带传播最终导致材料失效。     

Off-axis irradiation and the polarization of broad emission lines in active galactic nuclei

The stokes Monte Carlo radiative transfer code has been extended to model the velocity dependence of the polarization of emission lines. We use stokes to present improved modeling of the velocity-dependent polarization of broad emission lines in active galactic nuclei. We confirm that off-axis continuum emission can produce observed velocity dependencies of both the degree and position angle of polarization. The characteristic features are a dip in the percentage polarization and an S-shaped swing in the position angle of the polarization across the line profile. Some differences between our stokes results and previous modeling of polarization due to off-axis emission are noted. In particular we find that the presence of an offset between the maximum in line flux and the dip in the percentage of polarization or the central velocity of the swing in position angle does not necessarily imply that the scattering material is moving radially. Our model is an alternative scenario to the equatorial scattering disk described by Smith et al. (2005). We discuss strategies to discriminate between both interpretations and to constrain their relative contributions to the observed velocity-resolved line and polarization.     

Forest parameter estimation by means of Monte-Carlo simulations with experimental considerations – Estimation of multiple reflections among trees depending on forest parameters

A method for estimation of forest multiple light reflections depending on forest parameters is introduced, based on Monte-Carlo simulations of photon transport with experimental considerations. The model is verified through experiments with two miniature forests, in which two types of small-sized trees with ellipsoid- and cone-shaped crowns are arranged in a grid array. The introduced method was confronted with experimental measurements and showed small deviations from the measured values. It was found that the simulation of three-dimensional photon trajectories allowed a reliable evaluation of multiple light reflections among trees. In addition, the multiple reflections among trees due to the changes of tree inter-distance, crown type and crown shape were clarified with the proposed method.     

微吹气对湍流平板边界层流动特性的影响及其减阻机理

微吹气技术能够改变平板湍流流场结构,减小平板表面的摩擦阻力。采用直接数值模拟方法,计算了来流马赫数0.7条件下,流场流过光滑平板和NASA-PN2多孔平板表面两种情况,通过对比这两个算例的相关流场特征,验证了微吹气控制减阻的有效性,局部最大减阻率达到了45%,并且由于微吹气控制的"记忆"功能,减阻效果在微吹气流域下游仍会持续一段距离,增加了减阻区域的流向面积。壁湍流摩擦减阻的原因在于近壁区域出现了一个低速的"湍流斑",黏性底层厚度增加,速度型曲线被抬升。但与此同时,边界层内湍流速度脉动也得到了增强。进一步对流向脉动涡演化规律分析,发现微吹气对流向脉动涡发挥着多重作用。在增加流向脉动涡强度的同时,还使得流向涡团向远离壁面抬升,这样减小了流向涡与壁面之间直接作用。此外,微吹射流产生的冲击作用会在流向涡表面留下凹痕,使得流向涡分散成相对小的涡团结构。     

气密机身纵向裂纹非线性鼓胀因子数值研究

为了研究不同几何参数包括壳半径、壳壁厚度和裂纹长度对鼓胀因子的影响,应用有限元软件ABAQUS,通过几何非线性有限元分析,计算含纵向裂纹无加强柱形壳鼓胀因子的数值,并与现有的经验公式进行对比,同时讨论双轴载荷比对鼓胀因子的影响。结果表明:大部分几何参数对鼓胀因子的数值有显著影响;现有经验公式存在局限性;当双轴载荷比从0.5增长到1.0时,鼓胀影响降低了约20%;当双轴载荷比从0.5降低到0时,鼓胀影响增加了约28%。     

机场助航灯光光强动态检测系统

提出了一种机场助航灯光光强动态检测方法，该方法可以替代原有的人工巡检方式，实现快速、准确的在线检测灯光强度，发现灯光故障，保证飞机安全起降与滑行。系统采用安装在车体上的经余弦校正和v（λ）校正的条形照度传感带在水平面内动态扫描助航灯光发光截面，利用车载多普勒测距雷达测量距离，计算相应的光强值，并进而获得等光强图。为了保证系统的可靠性和测量精度，系统中采用了视频导航系统来保证检测车沿助航灯光中心线行驶，利用灯光定位传感器来消除测距雷达测量距离的累积误差。试验表明了该方法的可行性和检测精度。     

Revealing the hot intergalactic medium with ROSAT

The X-ray background intensity around galaxies and rich clusters of galaxies is investigated in three energy bands using the ROSAT All-Sky Survey maps. It is found that an amplitude of the XRB enhancements surrounding the Abell clusters and high density areas in the Lick galaxy counts depends on photon energy. Excess flux generated in the surrounding of the galaxy concentrations is consistent with the thermal emission by hot gas postulated by hydrodynamic simulations.     

1.5 MPa真空高压气淬炉快开结构应力计算

介绍了真空高压气淬炉炉门快开装置的主要结构，根据有关设计标准结合实际工作情况给出了1．5Mpa系列工程设计尺寸参数，采用ANSYS有限元软件分析了影响应力水平的主要因素，并以内径为1800mm的结构为例分析了简体、封头及卡箍圈的应力分布情况。     

Preliminary Study on Magnetic Induction Intensity Induced by Plasma During Hypervelocity Impact

An experimental system has been built to produce and measure the magnetic field in the backward ejected matter during hypervelocity impact. The designs of measurement system and coil, the choice of associated equipment, and the system calibration are also described in detail. The measurement of magnetic induction intensity for different given coil positions and azimuth angles are performed with two-stage light-gas gun. On condition that impact velocities are approximately equal and incidence angles are 45°, 60° and 90° respectively, the relationship between average magnetic induction intensity and impact angle at different time spans is obtained. Experimental results show that the average magnetic induction intensity with incidence angle of 90° is larger than those with incidence angles of 45°and 60°.