轴对称湍流射流的相似解

本文在相似性条件下,得到了用k-ε模式的轴对称湍流射流的相似方程。利用动量相似方程的近似求解结果作为初值,同时引入变量变换,进行迭代求解。本文的方法收敛速度快,计算简便。     

吸气条件对圆柱非定常分离流影响的数值研究

本文根据二维可压非定常Ｎ－Ｓ方程，基于Ｂｅａｍ ａｎｄ Ｗａｒｍｉｇｎ及Ｓｔｅｇｅｒ的方法，在圆柱绕流出现周期分离后，施加吸气条件，研究气对于圆柱非定常绕流的影响，计算结果表明，在恰当地区域施加恰当的吸气条件，可以希望通过减小压差阻力来减小总阻力，吸气还有抑制尾迹中非对称流动的作用，从而使圆柱所受的垂直于来流方向的升力的变化幅度减小，变化频率减小，但是吸气会增加磨擦阻力，过份的吸气会导致摩阻增大太     

A survey of radio jets with Chandra and HST

Relativistic jets are a common property of radio-loud Active Galactic Nuclei (AGN). Understanding jet physical properties is an essential precursor to understanding the mechanisms of energy transport, and ultimately, how energy is extracted from the central black hole. In this paper, I highlight recent developments from Chandra and HST observations of kpc-scale jets in AGN, with particular emphasis on our survey of 17 radio jets in a sample of FRII radio galaxies. These observations show that (1) X-ray and optical emission is common from kpc-scale jets, (2) a large fraction of the bolometric luminosity is emitted at X-rays, and (3) in most sources, a candidate emission process for the X-rays is inverse Compton scattering of the Cosmic Microwave Background off the relativistic electrons in the jet. If the latter scenario holds, the implication is that jets are still relativistic on kpc scales.     

Study of the variability of blazars gamma-ray emission

The γ-ray emission of blazar jets shows a pronounced variability and this feature provides limits to the size and to the speed of the emitting region. We study the γ-ray variability of bright blazars using data from the first 18 months of activity of the Large Area Telescope on the Fermi Gamma-Ray Space Telescope. From the daily light-curves of the blazars characterized by a remarkable activity, we firstly determine the minimum variability time-scale, giving an upper limit for the size of the emitting region of the sources, assumed to be spheroidal blobs in relativistic motion. These regions must be smaller than ∼10⁻³ parsec. Another interesting time-scale is the duration of the outbursts. We conclude that they cannot correspond to radiation produced by a single blob moving relativistically along the jet, but they are either the signature of emission from a standing shock extracting energy from a modulated jet, or the superposition of a number of flares occurring on a shorter time-scale. We also derive lower limits on the bulk Lorentz factor needed to make the emitting region transparent for gamma-rays interacting through photon–photon collisions.     

氩弧焊接方法对铝锂合金焊接接头性能和破坏的影响

介绍了几种氩弧焊方法对铝锂合金焊接接头性能和破坏断口特征的影响及其在不同铝锂合金焊件上的应用.     

D300mm×2000mm圆管内旋转流切向速度特征的实验研究

采用热线风速仪（HWA,Hot Wire Anemometry）测量了D300mm×2000mm圆管内旋转流切向瞬时速度随时间的变化特征。测量结果表明在圆管的中心区域,瞬时切向速度随时间的波动变化较大,而靠近边壁区域瞬时切向速度随时间的波动变化较小,中心区域瞬时切向速度的脉动幅值远大于壁面区域的脉动幅值。通过对瞬时切向速度进行频谱分析可知,瞬时切向速度的波动频率沿径向和轴向基本一致,但在出口区域频率有所增大,圆管内的瞬时切向速度出现低频波动是旋转流的摆动导致的。     

带圆孔加筋板的应力强度因子解析

采用Paris位移公式以及位移协调和叠加原理推导了求解带孔开裂加筋板的铆钉力计算式,并由此推导了只在孔边蒙皮上有裂纹和蒙皮开裂并在桁条上产生中心穿透次裂纹的两种开裂模态下的应力强度因子表达式,讨论了蒙皮与桁条的刚度比、铆钉间距以及裂纹扩展对裂尖应力强度因子的影响,得出了有参考价值的结果。     

Relativistic MHD Simulations of Jets with Toroidal Magnetic Fields

This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach.     

离心力场下细微封闭通道内R12的热驱动换热研究

本文以试验的方法,研究了一种利用彻体力场下封闭通道内流体的热驱动循环流动来强化换热的新型冷却技术。主要讨论了封闭循环通道宽度d为1mm,氟利昂R12为工质的热驱动流动和换热特性,重点分析了随转速(即离心加速度)的变化,R12的热驱动流动和换热变化规律,以及热端壁面的温度分布及变化规律。研究结果表明:离心力场下流体热驱动流动和换热特点同重力场下基本相似;随着转速的提高,R12的热驱动强度不断增加,热端壁面温度逐步下降,同时热端壁面的温度梯度也逐渐降低;在转速为1140r/min时,总平均传热系数达到了1550W/m2·K。