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Untitled - Aerobib - Universidad Politécnica de Madrid

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6.15. FLAME PROPAGATION IN HYDROGEN-BROMINE MIXTURES 193<br />

is the reduced activation temperature for the formation of HBr. These authors assume<br />

also that the coefficient of thermal conductivity λ is in<strong>de</strong>pen<strong>de</strong>nt of the composition<br />

of the mixture and that it varies proportionally with the square root of the temperature,<br />

viz.,<br />

λ = λ f<br />

√<br />

θ. (6.269)<br />

If Eqs. (6.266), (6.267), and (6.269) are introduced into Eq. (6.263), we obtain<br />

where<br />

dε 1<br />

dθ = X 3 X 3/2<br />

Λθ−1 2 (X 2 + 0.119X 1 ) −1 e −θ 1 − θ<br />

a<br />

θ<br />

, (6.270)<br />

θ − 1 + q 1 (ε 1f − ε 1 ) − q 4 (ε 4f − ε 4 )<br />

Λ = 1.6 × 10 14 λ ( ) 3/2<br />

f p<br />

m 2 M 1 e −θ a (6.271)<br />

c p RT f<br />

is the eigenvalue which <strong>de</strong>termines the propagation velocity u 0 of the flame through<br />

the relation<br />

u 0 = 1.265 × 10 7 1 ρ 0<br />

√<br />

λ f M 1<br />

c p<br />

( p<br />

RT f<br />

) 3/4<br />

e −θ a/2 Λ −1/2 . (6.272)<br />

The eigenvalue Λ can be obtained by applying the method of von Kármán<br />

and Penner [6] which involves integration of Eq. (6.270) between the cold and hot<br />

boundaries of the flame in the following form<br />

ε 2 ∫ ε1f (<br />

) ∫ 1<br />

1f<br />

q 1<br />

2 − X 3 X 3/2<br />

2 e −θ 1 − θ<br />

a<br />

θ<br />

1 − θ + q 4 (ε 4f − ε 4 ) dε 1 = Λ<br />

0<br />

θ 0<br />

θ(X 2 + 0.119X 1 )<br />

The problem lies now in obtaining:<br />

dθ. (6.273)<br />

1) Approximate expressions for (1 − θ) and (ε 4f − ε 4 ) as function of (ε 1f − ε 1 )<br />

for the computation on the integral on the left hand of Eq. (6.273).<br />

2) Approximate expressions for X 1 , X 2 , and X 3 as functions of θ, for the computation<br />

of the integral appearing on the right hand si<strong>de</strong>.<br />

Von Kármán and Penner [40] performed this computation by assuming that<br />

X 4 as well as ε 4 may be neglected (compared with unity). In this case, the diffusion<br />

equations (for Lewis number close to unity) show that X 1 , X 2 , and X 3 are linear<br />

functions of 1 − θ near θ = 1; a study of Eq. (6.270) shows that ε 1f − ε 1 is a function<br />

of θ of the form<br />

ε 1f − ε 1 = (1 − θ) n (6.274)

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