Polarizing gas at small optical depths around Algols

The origins of visible-band linear polarimetry of Algols and objects related to them are reviewed. It is pointed out, not for the first time, that the polarization signals of these systems can vary sporadically by significant amounts. The difficulty of evaluating the interstellar component of the observed polarization is discussed and these components are evaluated anew for each object studied in this paper. With one possible exception, the polarization signals intrinsic to these binaries derive from electron scattering. A well-defined model is applied to the constant and variable (but phase-locked) polarization signals. Limits to the mass associated with a scattering disk in each binary are derived. Within broad limits, concentrations of scattering mass within and above or below the orbital plane are also developed as are the centroid longitudes of these concentrations within the system. It is pointed out that very few measures of visible-band, circular polarization have been made but that cm-wavelength measures of Algol itself have been very informative.     

An optical and ultraviolet survey of Algols

We present a-table of results from our survey of Algols, conducted with the Lick Observatory ITS scanners and the IUE spectrometer.We have determined the continuous flux distributions for a number of the Algol systems. Optical scans were made with the ITS scanners of Lick Observatory, while for the ultraviolet flux distributions, we used the IUE satellite spectrometer in the low-dispersion mode. The following table summarizes the results: {ie340-01}     

Numerical simulation of a flow around airfoil using inviscid gas equations

A method for determining a field of inviscid gas equation application in finding the aerodynamic characteristics of bodies is proposed; as an example, use is made of airfoils for which extensive experimental data are available. The comparative analysis of physical and numerical simulation results showed a good verification of the method presented.     

天然气绕三角翼旋流的水洞实验研究

天然气绕三角翼产生旋流,使天然气中的游离水滴甩出,附着在管道内壁上,在气流的牵引下沿管道内壁向下游流动,实现了气水分离的目的。通过水洞实验,利用染色液流动显示技术,探讨了流体绕三角翼后产生旋流的可行性。同时,基于均匀设计思想对三角翼的前缘后掠角、后缘后掠角和迎角等几何参数分别做了5个水平的实验研究,均证实了天然气绕三角翼后产生旋流的可靠性,为该技术的应用奠定了基础。     

不同迎角下脊形前体绕流数值模拟研究

脊形前体有较强的背风涡流场,不同的前体形状对前体涡流场和气动力有很大的影响.本文针对脊形前体飞行器大迎角湍流大分离流动计算的困难,采用IDDES混合湍流模型,以及与之匹配的非定常算法,研究了不同来流迎角下脊形前体的气动特性,以及背风涡非定常演化、破裂的细致流动结构.选取了不同脊形角,以及不同上、下高宽比的脊形前体进行计...     

球形容器小口泄爆压力变化特性

以甲烷-空气预混气体为实验介质,研究了22L球形容器在小口有约束和无约束泄爆条件下,不同无量纲泄压比时的泄爆压力变化特性。研究发现：有约束泄爆时,当破膜压力保持不变,随着无量纲泄压比的减小,球形容器的最大泄爆压力和最大泄爆压力上升速率均增加;无量纲泄压比大于一定值时为平衡泄爆,否则为非平衡泄爆;有约束泄爆时,当无量纲泄压比大于0.009而小于0.025时,泄爆有着明显的效果,泄压是完全有效的;当无量纲泄压比大于0.00169而小于0.00900时,最大泄爆压力与密闭爆炸压力接近,泄爆效果较差;当无量纲泄压比小于0.00169时,最大泄爆压力略大于密闭状态下的爆炸压力;无约束泄爆时,不同无量纲泄压比的最大泄爆压力均低于密闭状态下的爆炸压力。实验结果为工业生产中球形容器的泄爆安全设计提供科学依据。     

低亚声速和跨声速矩形柱绕流的大涡模拟研究

采用基于非结构网格的有限体/有限元混合格式和大涡模拟的方法求解可压缩Navier-Stokes方程,研究了不同长宽比矩形柱低亚声速和跨声速绕流的流动特性。在雷诺数为22000时,对来流马赫数等于0.1和0.75,截面长宽比分别为1∶1、2∶1、3∶1和4∶1的矩形柱绕流进行了大涡模拟,以研究长宽比和压缩性对矩形柱绕流流场的影响。马赫数为0.1时,Strouhal数随着长宽比的增大先降低再增大然后再降低;长宽比为3∶1和4∶1时会有流动的再附产生;柱体上表面的三维特性在长宽比大时更明显。马赫数为0.75时,Strouhal数随着长宽比的增大逐渐减小;湍流脉动和涡脱落受到抑制;方柱的近尾迹区域,有两种形成机制不同的局部超声速区。     

多段翼型缝翼前缘结冰大迎角分离流动数值模拟

应用基于SST(Shear-Stress-Transport)湍流模型的IDDES(Improved Delayed Detached Eddy Simulation)方法,对大迎角状态下多段翼型缝翼前缘典型角状冰引起的复杂分离流动进行了数值模拟研究。采用后台阶流动标准算例和干净无冰多段翼型分离流动算例对数值方法的可靠性和适用性进行了验证。缝翼结冰状态下的数值模拟结果表明:来流迎角较大时,前缘角状冰将会导致结构相对稳定的流动分离泡产生,分离泡的非定常尾迹会对主翼前缘附近流场产生较为强烈的干扰,抑制了缝道流动的加速效应,使得缝翼增升效率降低。在失速点附近,由于分离泡回流强度随来流迎角而增长,同时脱落旋涡的输运方向逐渐向远离壁面方向偏移,使得尾迹影响区域范围和强度均有所增加。     

二元翼型大迎角绕流的平衡态(解)的数值研究

基于k-ω的SST两方程湍流模型,在时间域求解雷诺平均Navier-Stokes方程(RANS)计算了翼型大迎角分离流动.通过给翼型施加不同形式的扰动,重点关注了不同扰动形式对翼型大迎角分离涡流场平衡态的影响.研究表明:在所给定的百万雷诺数条件下,当翼型厚度达到一定程度而且在一定迎角范围内时,翼型的分离涡流场存在多个平衡态,且在一定扰动条件下会发生平衡态转移现象.在不同振动形式上,沉浮和俯仰比前后振动更易激发平衡态的转移.正是这种分离涡流场平衡态的多值现象,可能引发风洞实验中大迎角气动力数据的分散.     

Assessment of gas temperature fluctuations in the GTE combustion chamber exit section at generalizing experimental data on fuel combustion efficiency

It is suggested that gas composition at every point of the combustion chamber exit section be characterized by the temperature values T _i (“ideal” temperature) corresponding to the local values of the air-to-fuel coefficient α _i under complete fuel combustion (ν _comb ≈ 1). It is assumed that the values of T _i are distributed over the exit section area (gas mass) linearly and the values of T _imax and T _imin can be determined by the experimental data on the gas temperature fields in the combustion chambers. The distribution of temperatures T _i is used when it is necessary to generalize the experimental data on fuel combustion efficiency in GTE combustion chambers.