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Landau-Darrieus instability and the fractal dimension of flame fronts
90
Citations
26
References
1996
Year
Fractal StructureEngineeringFluid MechanicsCombustion TheoryLaminar FlamePremixed Turbulent FlameGas DynamicFractal ExcessNumerical SimulationFractal DimensionThermodynamicsNumerical SimulationsPhysicsTurbulent FlameNatural SciencesCombustion ScienceApplied PhysicsFractal AnalysisMultiscale Modeling
Nonlinear dynamics of a slow laminar flame front subject to the Landau-Darrieus instability is investigated by means of numerical simulations of the Frankel equation, when the expansion degree $\ensuremath{\gamma}=\frac{({\ensuremath{\rho}}_{u}\ensuremath{-}{\ensuremath{\rho}}_{b})}{{\ensuremath{\rho}}_{u}}$ is small (here ${\ensuremath{\rho}}_{u}$ and ${\ensuremath{\rho}}_{b}$ are the densities of the unburned and burned "gases," respectively). Only burning in two-dimensional space is considered in our simulations. The observed acceleration of a front wrinkled by the instability can be ascribed to the development of a fractal structure along the front surface with typical spatial scales being between the maximum and the minimum truly unstable wavelengths. It is found that the fractal excess $\ensuremath{\Delta}D=D\ensuremath{-}1$ decreases rapidly with decreasing of $\ensuremath{\gamma}$, to a first approximation as $\ensuremath{\Delta}D={D}_{0}{\ensuremath{\gamma}}^{2}$, where $D$ is the fractal dimension of the front. Our rough estimation of ${D}_{0}$ gives ${D}_{0}\ensuremath{\approx}0.3$. The low accuracy of the ${D}_{0}$ estimation is caused by certain peculiarities of the Frankel equation that lead to extreme difficulties of its simulation even with the aid of supercomputers when $\ensuremath{\gamma}\ensuremath{\lesssim}0.3\ensuremath{-}0.4$. It is shown, however, that ${D}_{0}$ can be calculated also from the statistical properties of the Sivashinsky equation, which is easier to simulate, though the fractal excess for the Sivashinsky equation itself is equal to 0 (in a certain sense). The other important result of our simulations is that the front self-intersections play an extremely weak role when $\ensuremath{\gamma}$ is small.
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