TY - JOUR
T1 - Ignition of combustible atmospheres caused by uniform and non-uniform radiation heating of an inert particle
AU - Stamatov, V.A.
AU - King, K.D.
AU - Zhang, Dongke
PY - 2006
Y1 - 2006
N2 - A modelling study of the ignition and explosion behaviour of quiescent methane/air mixtures caused by a radiatively heated inert particle has been carried out. Selecting the particle size much larger (about 2000 times) than the radiation wavelength reduces interference from Mie scattering. However, this results in axial non-symmetry of the processes of heat and mass transfer between, and within the particle and the surrounding gas phase. In order to simplify the model, the full number of space variables was reduced to one and a correlation factor between the cases of uniform and non-uniform radiative heating of the particle was established. The numerical simulations are compared with experimental results from previous studies. The theoretical predictions correlate well with the experimental values if the correlation factor is taken into account, however the absence of such a factor leads to significantly higher values (about 10 times) of the critical radiation power flux.
AB - A modelling study of the ignition and explosion behaviour of quiescent methane/air mixtures caused by a radiatively heated inert particle has been carried out. Selecting the particle size much larger (about 2000 times) than the radiation wavelength reduces interference from Mie scattering. However, this results in axial non-symmetry of the processes of heat and mass transfer between, and within the particle and the surrounding gas phase. In order to simplify the model, the full number of space variables was reduced to one and a correlation factor between the cases of uniform and non-uniform radiative heating of the particle was established. The numerical simulations are compared with experimental results from previous studies. The theoretical predictions correlate well with the experimental values if the correlation factor is taken into account, however the absence of such a factor leads to significantly higher values (about 10 times) of the critical radiation power flux.
UR - https://www.scopus.com/pages/publications/33646768178
U2 - 10.1080/00102200500325272
DO - 10.1080/00102200500325272
M3 - Article
SN - 0010-2202
VL - 178
SP - 1325
EP - 1344
JO - Combustion Science and Technology
JF - Combustion Science and Technology
IS - 7
ER -