超声速条件下多体干扰与分离试验研究

采用根据国外公开文献设计的类CAV模型,在0．6m×0．6m 跨/超声速风洞中开展了多体干扰与分离网格测力试验研究,初步获得了典型多体飞行器分离过程中的气动特性变化规律。试验结果表明,载荷模型气动特性受分离位置变化影响非常明显。载荷模型沿轴向分离时,气动力（矩）逐步接近自由流中气动力（矩）值,载荷模型法向位置改变会引发其气动力（矩）值发生更为剧烈的变化。引发这种现象的原因有两个：一是尾迹和头激波的发展改变了不同轴向位置处载荷模型的表面流态,从而影响了其气动特性;二是母机模型底部流动具有明显的非对称膨胀特征,不同法向位置处流速大小和方向差异明显,导致载荷模型气动特性随法向位置变化更为剧烈。     

Generalized Kutta–Joukowski theorem for multi-vortex and multi-airfoil flow(a lumped vortex model)

For purpose of easy identification of the role of free vortices on the lift and drag and for purpose of fast or engineering evaluation of forces for each individual body,we will extend in this paper the Kutta–Joukowski(KJ) theorem to the case of inviscid flow with multiple free vortices and multiple airfoils. The major simplification used in this paper is that each airfoil is represented by a lumped vortex,which may hold true when the distances between vortices and bodies are large enough. It is found that the Kutta–Joukowski theorem still holds provided that the local freestream velocity and the circulation of the bound vortex are modified by the induced velocity due to the outside vortices and airfoils. We will demonstrate how to use the present result to identify the role of vortices on the forces according to their position,strength and rotation direction. Moreover,we will apply the present results to a two-cylinder example of Crowdy and the Wagner example to demonstrate how to perform fast force approximation for multi-body and multi-vortex problems. The lumped vortex assumption has the advantage of giving such kinds of approximate results which are very easy to use. The lack of accuracy for such a fast evaluation will be compensated by a rigorous extension,with the lumped vortex assumption removed and with vortex production included,in a forthcoming paper.     

大型回流边界层风洞的气动与结构设计

大型边界层风洞是开展风工程研究的必备装备。以浙江大学ZD-1边界层风洞的研制为背景,详细介绍了大型回流边界层风洞气动设计和立式结构设计中的关键问题,在风洞气动设计时采用了收缩比为4∶1的单回路单试验段气动轮廓,在试验段中设置了0．22°的当量扩散角,对拐角导流片外形作了特殊处理,并采用钢结构与混凝土结构相结合的立式结构。流场校验结果表明,大型回流边界层风洞的气动与结构设计能满足设计要求,某些指标甚至达到航空风洞的标准,在试验段中设置扩散角有利于降低轴向静压梯度,立式结构设计对提高试验段气流的水平均匀性有一定的作用,可为今后类似风洞的研制提供参考。     

肋角度对气膜冷却特性的影响

在光滑二次流通道的基础上,分析对比了两种带肋通道(135°肋和45°肋)对气膜冷却特性的影响.采用瞬态液晶测试技术获得了气膜孔下游表面传热系数比与气膜冷却效率分布.使用Fluent软件RANS数值方法对相应结构进行了数值模拟,并使用了realizable k-ε湍流模型.光滑二次流通道模型中,气膜孔内流线呈螺旋状分布,导致较大的孔内速度分离与流动损失.冷气射流分成两部分,其中一股形成一对偏斜的对转涡.135°肋结构中,二次流通道上部分的旋转涡为顺时针方向,使得气流易于流入气膜孔,气膜孔内流线呈直线分布.45°肋结构中,二次流通道上部分旋转涡为逆时针方向,增强了气膜孔内旋转涡.45°肋结构中冷气流入气膜孔之后的流动结构与光滑二次流通道结构相似.135°肋结构气膜冷却效率最大而表面传热系数比最低.     

翼型舵面偏转非定常流动数值模拟

针对NACA0012翼型舵面偏转问题,数值模拟了不同参数对翼型气动特性的影响。基于非结构动网格技术,采用ALE有限体积描述下的二维可压缩非定常N-S方程,计算通量采用Vanleer格式、时空二阶格式,利用Venkatakrishnan限制器抑制数值振荡。非定常计算结果表明,NACA0012翼型绕1/4弦点作周期性俯仰振动的升力系数和俯仰力矩系数结果与实验数据吻合良好,验证了数值方法的准确性;在翼型舵面表面有分离区产生,升力系数和俯仰力矩系数形成滞回环,在亚声速情况下,滞回环幅值较小,进入超声速阶段以后,幅值增大,随着翼型间缝隙宽度逐渐增加,翼型升力系数和俯仰力矩系数与无缝翼型相比逐渐降低。     

螺旋桨瞬态流场数值模拟

建立完善的螺旋桨绕流理论异常困难,这一方面是由于螺旋桨流场整体旋转性、非定常非线性、三维效应、气流粘性、涡桨干扰等原因;另一方面是螺旋桨流场的流场结构有待于进一步认知。文章采用CFD方法对螺旋桨的瞬态流场结构进行了重点研究,详细绘制了自启动瞬间直至充分发展的螺旋桨瞬态流场结构图及所受气动力的变化图,分析了流场变化特性及其对升力的影响。     

现代民机新型灭火剂性能研究

对新型灭火剂研究背景和种类进行了简要介绍,对具有开发潜力的新型灭火剂的理化性能、毒性、腐蚀性、灭火性能、环保性能进行深入分析与研究。通过对新型灭火剂性能的研究,得出每种灭火剂的优缺点,筛选出适用于现代民机灭火系统的灭火剂。     

The ‘soot line’: Destruction of presolar polycyclic aromatic hydrocarbons in the terrestrial planet-forming region of disks

Interstellar material is highly processed when subjected to the physical conditions that prevail in the inner regions of protoplanetary disks, the potential birthplace of habitable planets. Polycyclic aromatic hydrocarbons (PAHs) are abundant in the interstellar medium, and they have also been observed in the disks around young stars, with evidence for some modification in the latter. Using a chemical model developed for sooting flames, we have investigated the chemical evolution of PAHs in warm (1000–2000 K) and oxygen-rich (C/O < 1) conditions appropriate for the region where habitable planets may eventually form. Our study focuses on (1) delineating the conditions under which PAHs will react and (2) identifying the key reaction pathways and reaction products characterizing this chemical evolution. We find that reactions with H, OH and O are the main pathways for destroying PAHs over disk timescale at temperatures greater than about 1000 K. In the process, high abundances of C₂H₂ persist over long timescales due to the kinetic inhibition of reactions that eventually drive the carbon into CO, CO₂ and CH₄. The thermal destruction of PAHs may thus be the cause of the abundant C₂H₂ that has been observed in disks. We propose that protoplanetary disks have a ‘soot line’, within which PAHs are irreversibly destroyed via thermally-driven reactions. The soot line will play an important role, analogous to that of the ‘snow line’, in the bulk carbon content of meteorites and habitable planets.     

赴美国、加拿大考察报告

介绍了赴美国国家标准与技术研究院。加拿大国家研究院等单位对化学计量进行考察的情况，浅谈了几点体会。     

全双工交换式千兆位以太网流量控制分析

分析了全双工效换式千兆位以太网流量控制策略，并在此基础上提出了提高网络性能的措施。