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Radiation affected laminar flame propagation.

机译:辐射影响层流火焰传播。

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The Rayleigh limit of the Lorenz-Mie theory is extended by the Penndorf expansion from {dollar}alpha{dollar} {dollar}cong{dollar} 0.3 to {dollar}alpha{dollar} {dollar}cong{dollar} 0.8, {dollar}alpha{dollar} being the particle size parameter. Error contours are generated for the Rayleigh and Penndorf limits for {dollar}alpha{dollar} = 0.3, 0.5 and 0.7 in the ranges 1.5 {dollar}leq{dollar} n {dollar}leq{dollar} 2.5 and 0.5 {dollar}leq{dollar} k {dollar}leq{dollar} 1.5 which cover the range of soot properties. The practical significance of the Penndorf extension is demonstrated in terms of optical diagnostics and radiative heat transfer. Also, the Planck and Rosseland mean absorption coefficients based on the Penndorf extension relative to those based on the Rayleigh limit are shown to depend on M's and N's which are explicit functions of the complex refractive index of particles, and on the fundamental dimensionless number {dollar}pi{dollar}DT/C{dollar}sb2{dollar} discovered in this study characterizing particulate matter--thermal radiation interaction (D being the particle diameter, T the temperature, and C{dollar}sb2{dollar} the second radiation constant). For larger particles and/or higher temperatures the Penndorf-based Planck mean coefficient is shown to deviate considerably from that of the Rayleigh-based coefficient. This deviation is exhibited to a somewhat lesser extent by the Penndorf-based Rosseland mean coefficient. The range of Penndorf-based coefficients are determined by accurate numerical computations utilizing the Lorenz-Mie theory. The computations are carried out by VASET, a computer code developed in this study.; Edwards' wide band model for discrete gas radiation is adopted, and a computer code, EMSVTY, has been developed in this study. The code improves the pure rotational band of water vapor, tabulates line width and optical depth parameters for 23 bands of 6 typical combustion species including H{dollar}sb2{dollar}O, CO{dollar}sb2{dollar}, CO, NO, SO{dollar}sb2{dollar}, and CH{dollar}sb4{dollar} from 200 K to 2500 K. It also demonstrates the relative significance of various gaseous species.; The effect of radiative losses on a freely propagating one-dimensional laminar premixed flame is investigated in terms of the flame speed, temperature profile, and the species concentrations. Detailed chemical kinetics (CHEMKIN) and transport (TRANFIT, TPINIT, etc.) algorithms are used in conjunction with PREMIX, a flame propagation code recently developed by Kee and coworkers at Sandia National Laboratories. The losses are shown to reduce the flame speed.
机译:Penndorf展开将{renal} alpha {dollar} {dollar} cong {dollar} 0.3扩展为{dollar} alpha {dollar} {dollar} cong {dollar} 0.8,{dollar},从而扩大了Lorenz-Mie理论的Rayleigh极限} alpha {dollar}是粒径参数。对于在1.5 {leqleq {dollar} n {dollar} leq {dollar} 2.5和0.5 {dollar} leq范围内的{dollar} alpha {dollar} = 0.3、0.5和0.7的Rayleigh和Penndorf极限,将生成误差轮廓。 {k} {q} {q} {q} {1.5}涵盖了烟尘特性的范围。 Penndorf扩展的实际意义在光学诊断和辐射热传递方面得到了证明。同样,基于Penndorf扩展的普朗克和Rosseland平均吸收系数相对于基于Rayleigh极限的平均吸收系数显示为取决于M和N,它们是颗粒的复数折射率的显函数,并且取决于基本的无量纲数{这项研究中发现的pi / pi / DT / Cb / sb2表征了热辐射的相互作用(D为粒径,T为温度,Cb / sb2为第二辐射)。不变)。对于较大的粒子和/或较高的温度,基于Penndorf的普朗克平均系数显示出与基于Rayleigh的系数大不相同。基于Penndorf的Rosseland平均系数在较小程度上显示了这种偏差。基于Penndorf系数的范围是通过利用Lorenz-Mie理论进行精确的数值计算确定的。计算是通过VASET进行的,VASET是本研究开发的计算机代码。采用了Edwards的离散气体辐射宽带模型,并在此研究中开发了计算机代码EMSVTY。该代码改善了水蒸气的纯旋转带,将6种典型燃烧物质的23个波段的线宽和光学深度参数制成表格,包括H {dollar} sb2 {dollar} O,CO {dollar} sb2 {dollar},CO,NO, SO {dollar} sb2 {dollar}和CH {dollar} sb4 {dollar}的范围为200 K至2500K。这也证明了各种气态物种的相对重要性。根据火焰速度,温度曲线和物质浓度,研究了辐射损失对自由传播的一维层流预混火焰的影响。详细的化学动力学(CHEMKIN)和运输(TRANFIT,TPINIT等)算法与PREMIX结合使用,PREMIX是由桑迪亚国家实验室的Kee和同事最近开发的火焰传播代码。损失表明降低了火焰速度。

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