Abstract

Flame extinction is one of the most essential critical flame features in combustion because of its relevance to combustion safety, efficiency, and pollutant emissions. In this paper, detailed simulations were conducted to investigate the effect of H2 addition on dimethyl ether spherical diffusion flame in microgravitational condition, in terms of flame structure, flammability, and extinction mechanism. The mole fraction of H2 in the fuel mixture was varied from 0 to 15% by 5% in increment. The chemical explosive mode analysis (CEMA) method was employed to reveal the controlling physicochemical processes in extinction. The results show that the cool flame in microgravitational diffusive geometry had the “double-reaction-zone” structure which consisted of rich and lean reaction segments, while the hot flame featured the “single-reaction-zone” structure. We found that the existence of “double-reaction-zone” was responsible for the stable self-sustained cool flame because the lean zone merged with the rich zone when the cool flame was close to extinction. Additionally, the effect of H2 addition on the cool flame was distinctively different from that of the hot flame. Both hot- and cool-flame flammability limits were significantly extended because of H2 addition but for different reasons. Besides, for each H2 addition case, the chemical explosive mode eigenvalues with the complex number appeared in the near-extinction zone, which implies the oscillation nature of flame in this zone which may induce extinction before the steady-state extinction turning point on the S-curve. Furthermore, as revealed by CEMA analysis, contributions of the most dominated species for extinction changed significantly with varying H2 additions, while contributions of the key reactions for extinction at varying H2 additions were basically identical.

Highlights

  • Studies on hydrocarbon fuel combustion are of great significance in improving flame stability, maximizing energy conversion efficiencies, and minimizing the environmental impacts of combustion systems.[1]

  • chemical explosive mode analysis (CEMA) which is based on the eigenanalysis of the Jacobian matrix of the chemical source term in governing equations is most useful in understanding the flame limit phenomena, and its effectiveness was verified in detecting the complicated interactions between chemistries in the multicomponent perfectly stirred reactor (PSR) combustion systems.[29,30]

  • Some representative hot flames and cool flames at various H2 addition cases were selected for examining the influence of H2 addition on the structure dynamics of the hot and cool spherical diffusion flame (SDF), respectively, and the results are shown in Figures 2 and 3

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Summary

INTRODUCTION

Studies on hydrocarbon fuel combustion are of great significance in improving flame stability, maximizing energy conversion efficiencies, and minimizing the environmental impacts of combustion systems.[1]. To identify critical flame features, including ignition, extinction, and stabilization mechanisms, some computational flame diagnostics such as sensitivity analysis,[24] computational singular perturbation (CSP),[25] and chemical explosive mode analysis (CEMA)[26−30] are proposed as systematic tools to extract important information from the simulation results, involved with the detailed chemical kinetic mechanism Among these diagnostic tools, CEMA which is based on the eigenanalysis of the Jacobian matrix of the chemical source term in governing equations is most useful in understanding the flame limit phenomena, and its effectiveness was verified in detecting the complicated interactions between chemistries in the multicomponent perfectly stirred reactor (PSR) combustion systems.[29,30] CEMA was employed for the present study

DESCRIPTIONS OF THE SIMULATIONS AND CEMA DIAGNOSTICS FORMULATIONS
RESULTS AND DISCUSSION
CONCLUSIONS
■ REFERENCES
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