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 ...
Chapter 2 Where, r c represents the local radius of the flame curvature. The first term of Eq. (2.21) represents the effect of the strain; the second term represents the effect of the fluid expansion of fluid (dilatation) and, the third term, the effect of the flame curvature. It is evident that the flame can be stretched by the combined effect of strain, volume expansion of the fluid and the curvature of the flame, which arises from the nonuniformities of the flow and the normal propagation of the flame front. For the present purposes, an appropriate unified tensor expression, in terms of strain rate, κ s , and the stretch rate due to flame curvature, κ c , is that of Candel and Poinsot, (1990). κ = κ + κ (2.22) s c tel-00623090, version 1 - 13 Sep 2011 With κ s =−nn: ∇ S+∇. S (2.23) κ = S ∇. n (2.24) c u In spherical expanding flames it is convenient to use spherical coordinates (r, θ, φ), the components of n and S are written as (n r , n θ , n φ ) and (s r , s θ , s φ ), respectively. Then: ⎡ 2⎛∂sr ⎞ 2⎛1 ∂s 2 1 s θ sr ⎞ ⎛ ∂ φ sr sθ cotθ ⎞ κs =− ⎢nr ⎜ n n r ⎟+ θ ⎜ + φ r θ r ⎟+ ⎜ + + ⎟ ⎣ ⎝ ∂ ⎠ ⎝ ∂ ⎠ ⎝r sinφ ∂φ r r ⎠ ⎛∂s 1 s s r s φ 1 s s θ ∂ θ ⎞ ⎛∂ ∂ r φ ⎞ + nn r θ ⎜ + − nn r φ r r θ r ⎟+ ⎜ + − ⎟ ⎝ ∂ ∂ ⎠ ⎝ ∂r r sinθ ∂φ r ⎠ ⎛1 ∂sφ 1 ∂sθ cotθ ⎞⎤ + nn θ φ ⎜ + − sφ ⎟⎥ ⎝r ∂θ r sinθ ∂φ r ⎠⎦⎥ 2 1 ∂ ( r sr ) 1 ∂ ( sθ sinθ ) 1 ∂sφ + + + 2 r ∂r r sinθ ∂θ r sinθ ∂ φ (2.25) 2 ( r nr ) ∂ ( n sinθ ) ⎡ 1 ∂ 1 1 ∂n ⎤ θ φ κc = un + ⎢ + + ⎥ 2 ⎢r ∂r r sinθ ∂θ r sinθ ∂φ ⎥ ⎣ ⎦ (2.26) For an outward spherically propagating flame, the flame surface is identified by the cold front of radius r u , n r =1, n θ =n φ =0, and s r =s g , s θ =s φ =0 (Bradley et al., 1996). The burning velocity, s u , is associated with this surface and the gas velocity ahead of it is s g . The flame speed, dr u /dt, is equal to s g + n r s u , and is indicated by S n . Applying this conditions to Eqs. 2.25 and 2.26 gives 45
Bibliographic revision 2 ( rsr ) 2 ⎛∂s ⎞ 1 ∂ κs = nr ⎜ + = ⎝ ∂ s r g 2 2 r ⎟ ⎠ r ∂r ru 2 ( r nr ) 1 ∂ s κc = un = 2n 2 r r ∂r r u u (2.27) (2.28) and the total stretch rate is: s κ = (2.29) 2 n ru The outwardly propagating flame, ignited from a central ignition point, is the most common spherical flame and because the stretch rates to which it is subjected are well defined, it is well suited to burning velocity measurements. tel-00623090, version 1 - 13 Sep 2011 2.5.1.1 Karlovitz number The Karlovitz number (Ka) is defined as the nondimensional stretch factor, using the thickness of the unstretched flame (δ u0 ) and the normal unstretched laminar flame velocity (S u0 ) to form a reference time (Kuo, 2005): Ka δ u0 = = (2.30) S u0 κ Residence time for crossing an unstretched flame Characteristic time for flame stretching For convenience, the Karlovitz number can be written as a sum of two parts due to the contribution from strain and curvature as follows: Ka = Ka + Ka (2.31) s c Where δ δ δ Ka = SS + : ∇ S ; Ka = S ∇ n = ( ηη) u 0 u 0 u 0 u s c u Su0 Su0 R Su0 S (2.32) 2.5.1.2 Markstein number Flame stretch can change the burning velocity of premixed flames significantly. It is important to know the relation between these two parameters, because the burning velocity is a crucial parameter in premixed combustion processes. Markstein, (1964) was the first to propose a phenomenological relation between the laminar burning velocity and the curvature of the flame front. Notice that the straining of the flow is not 46
- Page 1 and 2: THÈSE Pour l’obtention du Grade
- Page 3 and 4: Acknowledgements Acknowledgements T
- Page 5 and 6: Résumé __________________________
- Page 7 and 8: Nomenclature Nomenclature Roman tel
- Page 9 and 10: Nomenclature Subscripts tel-0062309
- Page 11 and 12: Contents tel-00623090, version 1 -
- Page 13 and 14: Contents 6.4. SYNGAS FUELLED-ENGINE
- Page 15 and 16: Introduction CHAPTER 1 INTRODUCTION
- Page 17 and 18: Introduction proves to have higher
- Page 19 and 20: Introduction Chapter 3 - Experiment
- Page 21 and 22: Bibliographic revision CHAPTER 2 BI
- Page 23 and 24: Bibliographic revision point today
- Page 25 and 26: Bibliographic revision - Boudouard
- Page 27 and 28: Bibliographic revision Table 2.1 -
- Page 29 and 30: Bibliographic revision Biomass Dryi
- Page 31 and 32: Bibliographic revision Circulating
- Page 33 and 34: Bibliographic revision or eliminate
- Page 35 and 36: Bibliographic revision established
- Page 37 and 38: Bibliographic revision Hydrogen Hyd
- Page 39 and 40: Bibliographic revision of low moist
- Page 41 and 42: Bibliographic revision scrubbing an
- Page 43 and 44: Bibliographic revision suggests tha
- Page 45 and 46: Bibliographic revision 1 d( δ A) 1
- Page 47: Bibliographic revision Since n is
- Page 51 and 52: Bibliographic revision This evoluti
- Page 53 and 54: Bibliographic revision The burning
- Page 55 and 56: Bibliographic revision δVG = − a
- Page 57 and 58: Bibliographic revision 2 1 − −
- Page 59 and 60: Bibliographic revision where the su
- Page 61 and 62: Bibliographic revision the stretche
- Page 63 and 64: Bibliographic revision burning velo
- Page 65 and 66: Experimental set ups and diagnostic
- Page 67 and 68: Experimental set ups and diagnostic
- Page 69 and 70: Experimental set ups and diagnostic
- Page 71 and 72: Experimental set ups and diagnostic
- Page 73 and 74: Experimental set ups and diagnostic
- Page 75 and 76: Experimental set ups and diagnostic
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- Page 81 and 82: Experimental set ups and diagnostic
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- Page 85 and 86: Experimental set ups and diagnostic
- Page 87 and 88: Experimental set ups and diagnostic
- Page 89 and 90: Chapter 4 CHAPTER 4 EXPERIMENTAL AN
- Page 91 and 92: Chapter 4 4.1 Laminar burning veloc
- Page 93 and 94: Chapter 4 4.1.1.1 Flame morphology
- Page 95 and 96: Chapter 4 P i = 1.0 bar, Ti = 293 K
- Page 97 and 98: Chapter 4 Figure 4.5 shows schliere
Chapter 2<br />
Where, r c represents the local radius of the f<strong>la</strong>me curvature. The first term of Eq. (2.21)<br />
represents the effect of the strain; the second term represents the effect of the fluid<br />
expansion of fluid (di<strong>la</strong>tation) and, the third term, the effect of the f<strong>la</strong>me curvature. It is<br />
evi<strong>de</strong>nt that the f<strong>la</strong>me can be stretched by the combined effect of strain, volume<br />
expansion of the fluid and the curvature of the f<strong>la</strong>me, which arises from the<br />
nonuniformities of the flow and the normal propagation of the f<strong>la</strong>me front.<br />
For the present purposes, an appropriate unified tensor expression, in terms of strain<br />
rate, κ s , and the stretch rate due to f<strong>la</strong>me curvature, κ c , is that of Can<strong>de</strong>l and Poinsot,<br />
(1990).<br />
κ = κ + κ<br />
(2.22)<br />
s<br />
c<br />
tel-00623090, version 1 - 13 Sep 2011<br />
With<br />
<br />
κ<br />
s<br />
=−nn: ∇ S+∇.<br />
S<br />
(2.23)<br />
κ = S ∇.<br />
n <br />
(2.24)<br />
c<br />
u<br />
In spherical expanding f<strong>la</strong>mes it is convenient to use spherical coordinates (r, θ, φ), the<br />
components of n and S are written as (n r , n θ , n φ ) and (s r , s θ , s φ ), respectively. Then:<br />
⎡<br />
2⎛∂sr ⎞ 2⎛1 ∂s<br />
2 1 s<br />
θ<br />
sr ⎞ ⎛ ∂<br />
φ sr<br />
sθ<br />
cotθ<br />
⎞<br />
κs<br />
=− ⎢nr<br />
⎜ n n<br />
r<br />
⎟+ θ ⎜ +<br />
φ<br />
r θ r<br />
⎟+ ⎜ + + ⎟<br />
⎣ ⎝ ∂ ⎠ ⎝ ∂ ⎠ ⎝r sinφ ∂φ<br />
r r ⎠<br />
⎛∂s<br />
1 s<br />
s<br />
r<br />
s<br />
φ 1 s s<br />
θ<br />
∂<br />
θ ⎞ ⎛∂<br />
∂<br />
r φ ⎞<br />
+ nn<br />
r θ ⎜ + − nn<br />
r φ<br />
r r θ r<br />
⎟+ ⎜ + − ⎟<br />
⎝ ∂ ∂ ⎠ ⎝ ∂r r sinθ ∂φ<br />
r ⎠<br />
⎛1 ∂sφ<br />
1 ∂sθ<br />
cotθ<br />
⎞⎤<br />
+ nn<br />
θ φ ⎜ + − sφ<br />
⎟⎥<br />
⎝r ∂θ r sinθ ∂φ<br />
r ⎠⎦⎥<br />
2<br />
1 ∂ ( r sr<br />
) 1 ∂ ( sθ<br />
sinθ<br />
) 1 ∂sφ<br />
+ +<br />
+<br />
2<br />
r ∂r<br />
r sinθ<br />
∂θ r sinθ ∂ φ<br />
(2.25)<br />
2<br />
( r nr<br />
) ∂ ( n sinθ<br />
)<br />
⎡ 1 ∂ 1 1 ∂n<br />
⎤<br />
θ<br />
φ<br />
κc<br />
= un<br />
+ ⎢ + + ⎥<br />
2<br />
⎢r<br />
∂r r sinθ ∂θ r sinθ ∂φ<br />
⎥<br />
⎣<br />
⎦<br />
(2.26)<br />
For an outward spherically propagating f<strong>la</strong>me, the f<strong>la</strong>me surface is i<strong>de</strong>ntified by the cold<br />
front of radius r u , n r =1, n θ =n φ =0, and s r =s g , s θ =s φ =0 (Bradley et al., 1996). The burning<br />
velocity, s u , is associated with this surface and the gas velocity ahead of it is s g . The<br />
f<strong>la</strong>me speed, dr u /dt, is equal to s g + n r s u , and is indicated by S n . Applying this conditions<br />
to Eqs. 2.25 and 2.26 gives<br />
45