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 H
2
addition on dimethyl
ether spherical diffusion flame in microgravitational condition, in
terms of flame structure, flammability, and extinction mechanism.
The mole fraction of H
2
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 H
2
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 H
2
addition but for different reasons.
Besides, for each H
2
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 H
2
additions, while
contributions of the key reactions for extinction at varying H
2
additions were basically identical.