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On the Formation of Nitrogen Oxides During the Combustion of ...

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4.2 Basics for Numerical Modeling<br />

4.2.2 Transport Mechanisms in <strong>the</strong> Gas Phase<br />

The species velocity difference ∆u m,r (i.e. <strong>the</strong> diffusion velocity) and <strong>the</strong> radial<br />

heat flux ˙q r can be derived from molecular gas kinetics [169, 180, 213], which<br />

is based on population dynamics. The distribution function<br />

f m (x, v m , t ) (4.7)<br />

is <strong>the</strong> number <strong>of</strong> molecules <strong>of</strong> species m per volume at position x with <strong>the</strong><br />

velocity vector v at time t . The bulk velocity<br />

∑ ∫<br />

n m n fn (x, v n , t )v n d v n<br />

u(x, t )= ∫ (4.8)<br />

∑n m n fn (x, v n , t ) d v n<br />

is calculated from <strong>the</strong> distribution function f n , with m n denoting <strong>the</strong> mass <strong>of</strong><br />

one molecule <strong>of</strong> species n. f m and f n are used similarly; <strong>the</strong> only difference is<br />

<strong>the</strong> name <strong>of</strong> <strong>the</strong> species – namely m or n. Thus, <strong>the</strong> species velocity is given by<br />

∫<br />

fm (x, v m , t )v m d v m<br />

u m (x, t )= ∫ . (4.9)<br />

fm (x, v m , t ) d v m<br />

Note that v m is <strong>the</strong> coordinate in <strong>the</strong> space-velocity frame, not <strong>the</strong> mean velocity<br />

<strong>of</strong> species m.<br />

After some rearranging [180], <strong>the</strong> diffusion velocity ∆u m,i can be calculated<br />

from Equation (4.9), with <strong>the</strong> bulk velocity u i in m s −1 , <strong>the</strong> velocity coordinate<br />

v m,i in m s −1 , <strong>the</strong> species density n m in m −3 , and <strong>the</strong> relation ρ = ∑ m n m m m .<br />

Employing ∆u m,i <strong>of</strong> Equation (4.10) to <strong>the</strong> energy (or heat flux) conservation<br />

equation and to <strong>the</strong> species conservation equation, it accounts for <strong>the</strong> Dufour<br />

and Soret effect, respectively. Both second-order effects are included in <strong>the</strong><br />

general derivations <strong>of</strong> this section but will be neglected in <strong>the</strong> final model, as<br />

outlined in Chapter 4.5.<br />

∆u m,i = 1 ∫ (vm,i )<br />

− u i fm dv m,i = 1 ∫<br />

∆v m,i f m d∆v m,i<br />

n m n m<br />

( n<br />

2 ∑<br />

=<br />

m n ˜D mn d m,i −<br />

n m ρ) D T (4.10)<br />

m ∂lnT<br />

n<br />

n m m m ∂x i<br />

The gradients in molar fraction X m = n m /n and in pressure p are summarized<br />

as vector d m,i according to Hirschfelder et al. [180] (see Eq. (4.11)). If <strong>the</strong> sys-<br />

121

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