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Untitled - Aerobib - Universidad Politécnica de Madrid

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3.8. STATIONARY, ONE-DIMENSIONAL MOTIONS 75<br />

3.8 Stationary, one-dimensional motions<br />

If the motion is not only one-dimensional but stationary, the preceding equations are<br />

consi<strong>de</strong>rably simplified. This type of motion, as previously stated, is of special interest<br />

for the study of the structure of combustion waves.<br />

The stationary motions are characterized by the condition<br />

∂ (·)<br />

= 0. (3.63)<br />

∂t<br />

Therefore, the only in<strong>de</strong>pen<strong>de</strong>nt variable is x.<br />

Let us see how the equations in the preceding paragraph can be simplified when<br />

condition (3.63) is introduced therein.<br />

Continuity Equations<br />

The continuity equation (3.49) reduces to<br />

v dρ<br />

dx + ρ dv<br />

dx ≡<br />

This equation can be integrated, thus obtaining<br />

d (ρv) = 0. (3.64)<br />

dx<br />

ρv = m, (3.65)<br />

where m is an integration constant which gives the mass flux per unit surface normal<br />

to the direction of motion.<br />

Similarly, equations (3.50) reduces to<br />

d<br />

dx (ρY iv + ρY i v di ) = w i , (i = 1, 2, . . . , l) . (3.66)<br />

By introducing the flux of the different species, these equations reduce to a<br />

very simple form. In fact, let m i = mε i be the flux of species A i through the unit<br />

surface normal to the direction of motion, that is to say that ε i is the fraction of the<br />

total flux corresponding to species A i . Since the velocity v i of species A i is<br />

v i = v + v di , (3.67)<br />

evi<strong>de</strong>ntly the said flux is<br />

mε i = ρY i (v + v di ) . (3.68)<br />

Now, when this expression is compared with the left hand si<strong>de</strong> of Eq. (3.66) it<br />

is seen that this system can be written in the form<br />

m dε i<br />

dx = w i, (i = 1, 2, . . . , l). (3.69)

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