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Syngas Mixture Composition Effects Upon Flashback and Blowout

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levels over which it was observed increasing with reactant<br />

preheat. As such, we postulated that this mechanism occurred<br />

when the turbulent flame speed exceeded some bulk or<br />

boundary layer flow velocity. However, results suggested that<br />

flashback can also occur even if the flame speed was never<br />

high enough to propagate upstream. In these instances, the<br />

flame can possibly manipulate the region of vortex breakdown<br />

by imposing an adverse pressure gradient ahead of the flame.<br />

This can explain the fact that the percentage of H 2 did not<br />

greatly affect the slow flashback limits since such a<br />

mechanism would be far less sensitive to the flame speed, but<br />

a strong function of the temperature ratio across the flame, as<br />

shown by these measurements.<br />

APPENDIX<br />

This appendix details a perturbation solution extracted<br />

from the Darrieus-L<strong>and</strong>au flame stability analysis † [35] for a<br />

flame with small sinusoidal wrinkles of spatial wavenumber k<br />

<strong>and</strong> amplitude D (see Figure 18), with flame temperature ratio<br />

R = T b /T u . The pressure upstream of the flame equals its<br />

nominal value, plus a small perturbation due to the wrinkle,<br />

'<br />

P(x) = P + P (x) . The acceleration of the gases through the<br />

flame causes the nominal burned gas pressure to drop, as<br />

given by the following expression:<br />

Figure 18: Schematic of flame front with small<br />

perturbation (Dashed line: x axis, Dot-dashed line: y axis).<br />

The dependence of this pressure rise upon the temperature<br />

ratio across the flame is plotted in Figure 19:<br />

2<br />

b<br />

=<br />

u<br />

− ( R − ) ρ (5)<br />

u u<br />

P P 1 U<br />

The alteration of the upstream pressure field by the flame<br />

wrinkle along the indicated line in the figure below is given by:<br />

'<br />

u ( ) −( R − )( σ − R)<br />

1 2<br />

( σ − 1)<br />

( ) [ ]<br />

u u<br />

2<br />

⎜<br />

⎝ σ + R<br />

where<br />

− R ⎡ 1 ⎤<br />

σ = ⎢ 1+ R + −1⎥<br />

1+ R ⎣ R ⎦<br />

kx<br />

P x 1 e<br />

=<br />

( ρ U )(kD) ⎛ ⎛ σ ⎞⎞<br />

2 R 1+ σ + ⎜1−<br />

⎟⎟<br />

⎝ R ⎠⎠<br />

The spatial dependence of the pressure through the flame<br />

along the dashed line in Figure 18 is plotted in Figure 14.<br />

The magnitude of the pressure rise upstream of the flame,<br />

indicated in Figure 14, is given by the expression:<br />

(6)<br />

(7)<br />

− ( R −1)( σ − R)<br />

( σ −1)<br />

( ) [ ] ⎛ σ ⎞<br />

⎟ ⎞<br />

1 + σ + ⎜ − ⎟<br />

σ + R<br />

R ⎠<br />

'<br />

∆P<br />

=<br />

⎛ ⎞ ⎛<br />

⎜<br />

1 ρ U<br />

2<br />

⎟( kD)<br />

u u 2⎜R<br />

1<br />

⎝ 2 ⎠ ⎝<br />

⎝<br />

† Note that this stability theory shows that such a<br />

perturbation is unstable. However, the corresponding pressure<br />

profiles are correct for the flame front whose instantaneous<br />

perturbation amplitude is D.<br />

⎠<br />

(8)<br />

Figure 19: Dependence of pressure rise upstream of the<br />

flame upon flame temperature ratio.<br />

This result shows that the adverse pressure gradient ahead<br />

of the flame grows monotonically with temperature ratio<br />

across the flame, as well as the relative inclination angle of the<br />

flame with respect to the flow, related to kD.<br />

ACKNOWLEDGEMENTS<br />

This publication was prepared with the support of the US<br />

Department of Energy, Office of Fossil Energy, National<br />

Energy Technology Laboratory, under contract 03-01-SR111<br />

<strong>and</strong> DE-FG26-04NT42176 (Dr. Richard Wenglarz <strong>and</strong> Ron<br />

Harp, contract monitors). Any opinions, findings,<br />

conclusions, or recommendations included herein are those of<br />

the authors <strong>and</strong> do not necessarily reflect the views of the<br />

DOE.<br />

10<br />

Copyright © 2006 by ASME

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