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The structure and extinction of a diffusion flame stabilized by a spherical porous burner, and attached to the burner, was analyzed by activation energy asymptotics.
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This work, while not experimental, does shows that radiative extinction of diffusion flames in a quiescent microgravity environment is possible.
Radiative extinction of spherical diffusion flames was investigated experimentally and numerically.
Extinction of counterflow diffusion flames of air and methane diluted with nitrogen is studied by drop tower experiments and numerical calculation using detailed chemistry transport properties.
These results corroborate the triple Forme stabiliftedon concept.
Therefore, it is concluded that extinction of spherical diffusion flame is primarily dictated by the local condition in the flame zone rather than by the volumetric radiative heat transfer in the surrounding gases.
The effects of radiation heat loss and variation in near-unity Lewis numbers on the structure and extinction of counterflow diffusion flame established near the stagnation plane of two opposed free streams of fuel and oxidizer are analyzed using the asymptotic method of large activation energy.
In particular, it is worth reporting that sufficiently small diffusion prevents the extinction of a whole system even if k SM is several times greater than k SP (e.g. if k SM = 1.7, k SP = 0.3, d = 0.001 and Δ = 0.01, then r ¯ ≈ 0.07).
This would require extensive numerical work, along with a derivation of a diffusion approximation to the mean extinction time for tight linkage.
Extinction of steady, spherical diffusion flames stabilized by a spherical porous burner was investigated by activation energy asymptotics.
Further increase of the rotation velocity results in abrupt extinction of the entire diffusion flame-ring at a critical and constant value of the Rossby number Roc = 7.
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