Burke–Schumann Flame
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In
combustion Combustion, or burning, is a high-temperature exothermic redox chemical reaction between a fuel (the reductant) and an oxidant, usually atmospheric oxygen, that produces oxidized, often gaseous products, in a mixture termed as smoke. Combusti ...
, a Burke–Schumann flame is a type of
diffusion flame In combustion, a diffusion flame is a flame in which the oxidizer and fuel are separated before burning. Contrary to its name, a diffusion flame involves both diffusion and convection processes. The name diffusion flame was first suggested by S. ...
, established at the mouth of the two concentric ducts, by issuing fuel and oxidizer from the two region respectively. It is named after S.P. Burke and T.E.W. Schumann, who were able to predict the flame height and flame shape using their simple analysis of infinitely fast chemistry (which is now called as
Burke–Schumann limit In combustion, Burke–Schumann limit, or large Damköhler number limit, is the limit of infinitely fast chemistry (or in other words, infinite Damköhler numbers, Damköhler number), named after S.P. Burke and T.E.W. Schumann, due to their pioneeri ...
) in 1928 at the First symposium on combustion.


Mathematical description

Consider a cylindrical duct with axis along z direction with radius a through which fuel is fed from the bottom and the tube mouth is located at z=0. Oxidizer is fed along the same axis, but in the concentric tube of radius b outside the fuel tube. Let the mass fraction in the fuel tube be Y_ and the mass fraction of the oxygen in the outside duct be Y_. Fuel and oxygen mixing occurs in the region z>0. The following assumptions were made in the analysis: * The average velocity is parallel to axis (z direction) of the ducts, \mathbf= v \mathbf_z *The mass flux in the axial direction is constant, \rho v=\mathrm *Axial diffusion is negligible compared to the transverse/radial diffusion * The flame occurs infinitely fast (
Burke–Schumann limit In combustion, Burke–Schumann limit, or large Damköhler number limit, is the limit of infinitely fast chemistry (or in other words, infinite Damköhler numbers, Damköhler number), named after S.P. Burke and T.E.W. Schumann, due to their pioneeri ...
), therefore flame appears as a reaction sheet across which properties of flow changes * Effects of gravity has been neglected Consider a one-step irreversible
Arrhenius law In physical chemistry, the Arrhenius equation is a formula for the temperature dependence of reaction rates. The equation was proposed by Svante Arrhenius in 1889, based on the work of Dutch chemist Jacobus Henricus van 't Hoff who had noted in 1 ...
, \mathrm+s\mathrm_2\rightarrow (1+s)\mathrm+q, where s is the mass of oxygen required to burn unit mass of fuel and q is the amount of heat released per unit mass of fuel burned. If \omega is the mass of fuel burned per unit volume per unit time and introducing the non-dimensional fuel and mass fraction and the Stoichiometry parameter, :y_F = \frac,\quad y_O = \frac,\quad S = \frac the governing equations for fuel and oxidizer mass fraction reduce to :\begin \frac\frac\left(r\frac\right) - \rho v\frac = \frac \\ \frac\frac\left(r\frac\right) - \rho v\frac = S\frac \\ \end where
Lewis number The Lewis number (Le) is a dimensionless number defined as the ratio of thermal diffusivity to mass diffusivity. It is used to characterize fluid flows where there is simultaneous heat and mass transfer. The Lewis number puts the thickness of the th ...
of both species is assumed to be unity and \rho D_T is assumed to be constant, where D_T is the
thermal diffusivity In heat transfer analysis, thermal diffusivity is the thermal conductivity divided by density and specific heat capacity at constant pressure. It measures the rate of transfer of heat of a material from the hot end to the cold end. It has the SI ...
. The boundary conditions for the problem are :\begin \text\, &z=0,\, 0 The equation can be linearly combined to eliminate the non-linear reaction term \omega/Y_ and solve for the new variable :Z = \frac, where Z is known as the mixture fraction. The mixture fraction takes the value of unity in the fuel stream and zero in the oxidizer stream and it is a scalar field which is not affected by the reaction. The equation satisfied by Z is :\frac\frac\left(r\frac\right) - \frac\frac=0 (If the Lewis numbers of fuel and oxidizer are not equal to unity, then the equation satisfied by Z is nonlinear as follows from Shvab–Zeldovich–Liñán formulation). Introducing the following coordinate transformation :\xi = \frac, \quad \eta = \frac \frac, \quad c= \frac reduces the equation to :\frac\frac\left(\xi\frac\right) - \frac=0. The corresponding boundary conditions become :\begin \text\, &\eta=0,\, 0<\xi The equation can be solved by separation of variables :Z(\xi,\eta) = c^2 + 2c \sum_^\infty \frac \frac J_0(\lambda_n \xi)e^ where J_0 and J_1 are the
Bessel function of the first kind Bessel functions, first defined by the mathematician Daniel Bernoulli and then generalized by Friedrich Bessel, are canonical solutions of Bessel's differential equation x^2 \frac + x \frac + \left(x^2 - \alpha^2 \right)y = 0 for an arbitrary ...
and \lambda_n is the nth root of J_1(\lambda)=0. Solution can also be obtained for the planar ducts instead of the axisymmetric ducts discussed here. Williams, F. A. (1965). Combustion Theory: the fundamental theory of chemical reacting flow systems. Addison-Wesley.


Flame shape and height

In the Burke-Schumann limit, the flame is considered as a thin reaction sheet outside which both fuel and oxygen cannot exist together, i.e., y_Fy_O=0. The reaction sheet itself is located by the stoichiometric surface where Sy_F=y_O, in other words, where :Z=Z_s \equiv \frac where Z_s is the stoichiometric mixture fraction. The reaction sheet separates fuel and oxidizer region. The inner structure of the reaction sheet is described by Liñán's equation. On the fuel side of the reaction sheet (Z>Z_s) :y_F = \frac,\, y_O=0 and on the oxidizer side (Z) :y_F=0,\, y_O = 1-\frac. For given values of Z_s (or, S) and c, the flame shape is given by the condition Z(\xi,\eta)=Z_s, i.e., :Z_s=c^2 + 2c \sum_^\infty \frac \frac J_0(\lambda_n \xi)e^. When Z_s\rightarrow 0 (S\rightarrow \infty), the flame extends from the mouth of the inner tube and attaches itself to the outer tube at a certain height (under-ventilated case) and when Z_s\rightarrow 1 (S\rightarrow 0), the flame starts from the mouth of the inner tube and joins at the axis at some height away from the mouth (over-ventilated case). In general, the flame height is obtained by solving for \eta in the above equation after setting \xi=1 for the under-ventilated case and \xi=0 for the over-ventilated case. Since flame heights are generally large for the exponential terms in the series to be negligible, as a first approximation flame height can be estimated by keeping only the first term of the series. This approximation predicts flame heights for both cases as follows :\begin \eta &= \frac\ln \left frac\right\quad \text \\ \eta &= \frac\ln \left frac\right\quad \text, \end where \lambda_1=3.8317.


References

{{DEFAULTSORT:Burke-Schumann flame Fire Combustion Fluid dynamics