Numerical investigation to evaluate the effects of gravity and pressure on flame structure and soot formation of turbulent non-premixed methane-air flame

IF 5.4 2区 工程技术 Q1 ENGINEERING, AEROSPACE
Subrat Garnayak , Amjad Ali Pasha , Radi Alsulami , Medhat A. Nemitallah , Abdul Gani Abdul Jameel , Sukanta K. Dash , V. Mahendra Reddy
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引用次数: 2

Abstract

In this study, a turbulent non-premixed (diffusion) methane-air flame has been investigated computationally to analyze the influences of pressure and gravity on flame structure and sooting characteristics between 1 and 10 atm. The simulation has been conducted in a 2-D axisymmetric computational domain using the finite volume-based computational fluid dynamics (CFD) code. The interaction of turbulence and chemistry is modeled by considering the steady laminar flamelet model (SLFM) and the GRI Mech 3.0 chemical mechanism. The radiative heat transfer calculation is carried out by considering the discrete ordinate (DO) method and the weighted sum grey gas model (WSGGM). The semi-empirical Moss-Brookes model is considered to calculate soot. The impact of gravity on flame and sooting characteristics are evaluated by comparing the normal-gravity flames with the zero-gravity flames. The effect of soot and radiation on flame temperature is also examined. The results show a close agreement with the measurement when both soot and radiation are included in the numerical modeling. The rates of soot formation, surface growth, and oxidation increase with increased operating pressure, regardless of gravity. Zero-gravity flames have a higher soot volume fraction, a wider soot-containing zone, a higher CO mass fraction, and a lower flame temperature than normal-gravity flames while maintaining constant pressure. In normal-gravity flames, the CO mass fraction decreases with pressure, whereas it increases with pressure rise in flames of zero gravity. Flames of zero gravity appear taller and broader compared to the flames of normal-gravity for a fixed pressure. An increase in pressure significantly reduces the flame length and width in normal-gravity flames. However, the pressure elevation has little effect on the shape of a zero-gravity flame. The outcomes of the present study will assist in fully understanding the combustion and sooting characteristics of turbulent diffusion flames that will help design and develop high-efficiency, pollutant-free combustion devices and fire suppression systems for space application.

重力和压力对湍流非预混甲烷-空气火焰火焰结构和烟尘形成影响的数值研究
本文对一种湍流非预混(扩散)甲烷-空气火焰进行了计算研究,分析了压力和重力在1 ~ 10atm范围内对火焰结构和散烟特性的影响。利用基于有限体积的计算流体力学(CFD)程序在二维轴对称计算域中进行了数值模拟。考虑稳定层流小火焰模型(SLFM)和GRI Mech 3.0化学机理,建立了湍流与化学相互作用的模型。采用离散坐标法(DO)和加权和灰气模型(WSGGM)进行辐射传热计算。采用半经验Moss-Brookes模型计算烟尘。通过对正常重力火焰和零重力火焰的比较,评估了重力对火焰和烟气特性的影响。研究了烟尘和辐射对火焰温度的影响。当数值模拟中同时考虑烟尘和辐射时,计算结果与实测结果吻合较好。无论重力如何,随着操作压力的增加,烟灰形成、表面生长和氧化的速率都会增加。在恒压条件下,零重力火焰比正重力火焰具有更高的烟尘体积分数、更宽的含烟区、更高的CO质量分数和更低的火焰温度。在正常重力火焰中,CO质量分数随压力的增大而减小,而在零重力火焰中,CO质量分数随压力的增大而增大。与固定压力下的正常重力火焰相比,零重力火焰显得更高更宽。压力的增加显著地减少了正常重力火焰的火焰长度和宽度。而压力标高对零重力火焰的形状影响不大。本研究的结果将有助于充分了解湍流扩散火焰的燃烧和烟尘特性,这将有助于设计和开发用于空间应用的高效,无污染的燃烧装置和灭火系统。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
7.50
自引率
5.70%
发文量
30
期刊介绍: Propulsion and Power Research is a peer reviewed scientific journal in English established in 2012. The Journals publishes high quality original research articles and general reviews in fundamental research aspects of aeronautics/astronautics propulsion and power engineering, including, but not limited to, system, fluid mechanics, heat transfer, combustion, vibration and acoustics, solid mechanics and dynamics, control and so on. The journal serves as a platform for academic exchange by experts, scholars and researchers in these fields.
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