Etude de la combustion de gaz de synthèse issus d'un processus de ...

Etude de la combustion de gaz de synthèse issus d'un processus de ... Etude de la combustion de gaz de synthèse issus d'un processus de ...

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Chapter 2 Where r b is the radius of the inner boundary of the unburned gas of density ρ u . Combining the above relations results in −1 dp Ab ρu ⎛dx ⎞ = ⎜ ⎟ S dt V ρi ⎝dp ⎠ u (2.56) Isentropic compression of the unburned gases gives ρ ⎛ u p ⎞ = ⎜ ⎟ ρi ⎝pi ⎠ −1 γ u (2.57) Or, alternatively, tel-00623090, version 1 - 13 Sep 2011 ( γu −1) γu ⎛ p ⎞ Tu = Ti ⎜ ⎟ p i ⎝ ⎠ . (2.58) Where γ u = c pu /c vu , is the isentropic exponent of the unburned mixture. Surface area and volume of the flame are related to its radius as A b = 4πr 2 and Vb 4 3 = π r , 3 respectively. Realizing that m u = ρ i V (1 − x), and p i = ρ i R u T i , the volume of the unburned mixture can be written as Inserting Vb V=V u +V b yields: V mRT p T ( 1 ) = u u u i u u X V p = p T − (2.59) i 4 3 = πR , R is the effective radius of the vessel and the above relations into 3 pi Tu rb R ⎡ ⎤ = ⎢1−( 1−x) ⎥ ⎣ pT i ⎦ 1/ 3 (2.60) The area-to-volume ratio in Eq. (2.56) now becomes: A 3 ⎡ b p 1 ( 1 i T ⎤ u = ⎢ − −x) ⎥ V R ⎣ p Ti ⎦ 2/3 (2.61) Inserting Eqs. (2.57), (2.58) and (2.61) into Eq.(2.56) we finally obtain 53

Bibliographic revision 2 1 − − ⎤ 3 γu −1 ⎡ dp 3 ⎛dx ⎞ ⎛ pi ⎞ ⎛ p ⎞ = ⎢1 ( 1 x) ⎥ ⎜ ⎟ −⎜ ⎟ − ⎜ ⎟ dt R ⎝dp ⎠ ⎢ ⎝ p ⎠ ⎥ ⎝ pi ⎢ ⎥ ⎠ ⎣ ⎦ 1 − γu S u (2.62) A result first derived by O´Donovan and Rallis, (1959). Rearranging Eq. (2.62) gives: S u 2 1 − ⎤ 3 γu 1 ⎡ − R⎛dx ⎞ ⎛p u i ⎞ ⎛ p ⎞ γ ⎛dp⎞ = ⎢1 ( 1 x) ⎥ ⎜ ⎟ − − 3 dp ⎢ ⎜ ⎟ ⎜ ⎟ p ⎥ p ⎜ i dt ⎟ ⎝ ⎠ ⎝ ⎠ ⎝ ⎠ ⎝ ⎠ ⎢⎣ ⎥⎦ (2.63) tel-00623090, version 1 - 13 Sep 2011 In this equation, R is the effective radius of the vessel and γ u = c pu /c vu , the isentropic exponent of the unburned mixture. Both x and its derivative dx/dp depend on pressure. The advantage of this expression of the burning velocity is the possibility of exploring a wide range of pressures and temperatures with one explosion. This is the main reason of its utilization for burning velocity determination in engine conditions. Several x(p) relations have been proposed in the literature. The most important of which are: - O’Donovan and Rallis (1959) Based on the same assumptions mentioned, O’Donovan and Rallis (1959) present an x(p) relation that in the present symbols reads, ( γu −1)/ ( / i ) ( ) p− pi( Tu / Ti) T ⎛ p− p e i p p x = = pe( Tb / Te) − pi( Tu / Ti) T ⎜ b ⎝pe − ( Tb / Te) pi p/ pi γu ( γu −1)/ γu ⎞ ⎟ ⎠ (2.64) Tb is the mass averaged burnt temperature during combustion, with end value T e . T b is determined for every burned shell from 3 consecutive increases. First its unburned temperature is determined from adiabatic compression. Its burned temperature is then obtained from energy conservation for the shell at constant pressure. Finally, the burned shell is further compressed (and heated) adiabatically. As a further simplification to their model, O’Donovan and Rallis assume that Tb and T e are equal during the whole combustion period. In this case one finds p− pi( p/ pi) x = p − p ( p/ p ) ( γu −1)/ γu ( γu −1)/ γu e i i (2.65) 54

Bibliographic revision<br />

2<br />

1<br />

−<br />

− ⎤ 3<br />

γu<br />

−1<br />

⎡<br />

dp 3 ⎛dx ⎞ ⎛ pi<br />

⎞<br />

⎛ p ⎞<br />

= ⎢1 ( 1 x)<br />

⎥<br />

⎜ ⎟ −⎜ ⎟ − ⎜ ⎟<br />

dt R ⎝dp ⎠ ⎢ ⎝ p ⎠ ⎥<br />

⎝ pi<br />

⎢<br />

⎥<br />

⎠<br />

⎣<br />

⎦<br />

1<br />

−<br />

γu<br />

S<br />

u<br />

(2.62)<br />

A result first <strong>de</strong>rived by O´Donovan and Rallis, (1959). Rearranging Eq. (2.62) gives:<br />

S<br />

u<br />

2<br />

1<br />

−<br />

⎤ 3<br />

γu<br />

1<br />

⎡<br />

−<br />

R⎛dx ⎞ ⎛p<br />

u<br />

i<br />

⎞ ⎛ p ⎞ γ<br />

⎛dp⎞<br />

= ⎢1 ( 1 x)<br />

⎥<br />

⎜ ⎟ − −<br />

3 dp ⎢ ⎜ ⎟ ⎜ ⎟<br />

p ⎥ p<br />

⎜<br />

i<br />

dt<br />

⎟<br />

⎝ ⎠ ⎝ ⎠ ⎝ ⎠ ⎝ ⎠<br />

⎢⎣<br />

⎥⎦<br />

(2.63)<br />

tel-00623090, version 1 - 13 Sep 2011<br />

In this equation, R is the effective radius of the vessel and γ u = c pu /c vu , the isentropic<br />

exponent of the unburned mixture. Both x and its <strong>de</strong>rivative dx/dp <strong>de</strong>pend on pressure.<br />

The advantage of this expression of the burning velocity is the possibility of exploring a<br />

wi<strong>de</strong> range of pressures and temperatures with one explosion. This is the main reason<br />

of its utilization for burning velocity <strong>de</strong>termination in engine conditions. Several x(p)<br />

re<strong>la</strong>tions have been proposed in the literature. The most important of which are:<br />

- O’Donovan and Rallis (1959)<br />

Based on the same assumptions mentioned, O’Donovan and Rallis (1959) present an<br />

x(p) re<strong>la</strong>tion that in the present symbols reads,<br />

( γu<br />

−1)/<br />

( /<br />

i )<br />

( )<br />

p−<br />

pi( Tu / Ti)<br />

T ⎛ p−<br />

p<br />

e<br />

i<br />

p p<br />

x = =<br />

pe( Tb / Te) − pi( Tu / Ti) T ⎜<br />

b<br />

⎝pe − ( Tb / Te) pi p/<br />

pi<br />

γu<br />

( γu<br />

−1)/<br />

γu<br />

⎞<br />

⎟<br />

⎠<br />

(2.64)<br />

Tb<br />

is the mass averaged burnt temperature during <strong>combustion</strong>, with end value T<br />

e<br />

. T b is<br />

<strong>de</strong>termined for every burned shell from 3 consecutive increases. First its unburned<br />

temperature is <strong>de</strong>termined from adiabatic compression. Its burned temperature is then<br />

obtained from energy conservation for the shell at constant pressure. Finally, the<br />

burned shell is further compressed (and heated) adiabatically.<br />

As a further simplification to their mo<strong>de</strong>l, O’Donovan and Rallis assume that Tb<br />

and T<br />

e<br />

are equal during the whole <strong>combustion</strong> period. In this case one finds<br />

p−<br />

pi( p/ pi)<br />

x =<br />

p − p ( p/ p )<br />

( γu<br />

−1)/<br />

γu<br />

( γu<br />

−1)/<br />

γu<br />

e i i<br />

(2.65)<br />

54

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