TY - JOUR
T1 - Effects of radiation heat loss on the flammable region of counterflow premixed flames at a large Lewis number
AU - Ju, Yiguang
AU - Guo, Hongsheng
AU - Maruta, Kaoru
PY - 1997
Y1 - 1997
N2 - The extinction limits and flammable regions of a nonadiabatic counterflow premixed flame at a large Lewis number are investigated numerically. It is found that interaction between the radiative heat loss and the Lewis number effect results in four kinds of flame bifurcations. Furthermore, the results show that there exist four different kinds of flame regimes: normal flames, radiation-stretch-induced weak flames, radiation Lewis number effect-induced weak flames and unified weak flames at typical equivalence ratios. An increase in the radiation intensity reduces the extinction limit of a normal flame but extends the flammable region of weak flames to large stretch rates. A general graph showing the extinction limits and the flammable regions is obtained. It is found that the G-shaped curve obtained at a low Lewis number is reduced to a K-shaped curve at a large Lewis number. This G-K transition presents a good explanation for the experimental results obtained in microgravity experiments.
AB - The extinction limits and flammable regions of a nonadiabatic counterflow premixed flame at a large Lewis number are investigated numerically. It is found that interaction between the radiative heat loss and the Lewis number effect results in four kinds of flame bifurcations. Furthermore, the results show that there exist four different kinds of flame regimes: normal flames, radiation-stretch-induced weak flames, radiation Lewis number effect-induced weak flames and unified weak flames at typical equivalence ratios. An increase in the radiation intensity reduces the extinction limit of a normal flame but extends the flammable region of weak flames to large stretch rates. A general graph showing the extinction limits and the flammable regions is obtained. It is found that the G-shaped curve obtained at a low Lewis number is reduced to a K-shaped curve at a large Lewis number. This G-K transition presents a good explanation for the experimental results obtained in microgravity experiments.
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U2 - 10.1299/kikaib.63.4069
DO - 10.1299/kikaib.63.4069
M3 - Article
AN - SCOPUS:0031360943
SN - 0387-5016
VL - 63
SP - 255
EP - 261
JO - Nippon Kikai Gakkai Ronbunshu, B Hen/Transactions of the Japan Society of Mechanical Engineers, Part B
JF - Nippon Kikai Gakkai Ronbunshu, B Hen/Transactions of the Japan Society of Mechanical Engineers, Part B
IS - 616
ER -