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simulation of offgas scrubbing by a combined eulerian ... - CFD

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The force balance for a single dust particle can be written<br />

as<br />

2<br />

ρ Pu<br />

Drift 24<br />

mPu&<br />

P = mP<br />

g − A .<br />

P<br />

2 Re<br />

Using the particle relaxation time,<br />

Copyright © 2009 CSIRO Australia 4<br />

τ<br />

P<br />

ρ d<br />

2<br />

P P<br />

P,<br />

relax = ,<br />

18μG<br />

above equation can be written as<br />

u& u Drift<br />

= g − . (7)<br />

P<br />

τ<br />

P,<br />

relax<br />

Assuming local equilibrium one can assume that:<br />

∂uG<br />

u& P = + ( ∇ ⋅u<br />

G ) u (8)<br />

G<br />

∂t<br />

Thus, using equations (7) and (8) the drift velocity can be<br />

calculated from the gas velocity and the particle<br />

properties.<br />

The dispersion <strong>of</strong> particles strongly depends on the<br />

turbulence structure. According to Crowe (1985), the<br />

reciprocal Schmidt number denoting the ratio <strong>of</strong><br />

diffusivity and effective viscosity is a function <strong>of</strong> the time<br />

τ τ ,<br />

ratio P , relax G,<br />

turb<br />

Ddiff<br />

ρG<br />

⎛τ<br />

⎞ P,<br />

relax<br />

= F⎜<br />

⎟ . (9)<br />

η ⎜ ⎟<br />

G ⎝ τ G,<br />

turb ⎠<br />

Here<strong>by</strong>, in RANS <strong>simulation</strong>s using the k-ε turbulence<br />

model the characteristic time <strong>of</strong> large scale turbulent<br />

structures can be approximated as<br />

τ<br />

k<br />

0.<br />

15<br />

ε<br />

G,<br />

turb = . (10)<br />

Thus, using above correlation the dust phases diffusivity<br />

can be calculated from turbulence parameters and the dust<br />

particles’ relaxation time.<br />

Modelling the capture <strong>of</strong> dust particles<br />

As Hähner (1994) pointed out, there are at least three<br />

mechanisms that might lead to deposition <strong>of</strong> dust particles<br />

(Figure 3) diffusion, impaction and interception.<br />

Figure 3: Principle dust capturing mechanisms occurring<br />

in a Venturi scrubber.<br />

In principle all these mechanisms occur simultaneously,<br />

but depending on the size ratio and the relative velocity<br />

between dust and droplet they become more or less<br />

important. At high relative velocities, as they occur in<br />

Venturi scrubbers, and micron sized dust particles,<br />

impaction is the dominant capturing mechanism while for<br />

smaller dust particles diffusion becomes more important<br />

(Kim, 2001).<br />

Impaction<br />

In literature many correlations for inertial drop collection<br />

efficiency are available (e.g. Pak, 2006; Pulley, 1997; Kim<br />

2001). As a dimensionless number characterizing inertial<br />

collection a modified Stokes number is used,<br />

ψ<br />

ρ d<br />

u − u<br />

=<br />

P<br />

2<br />

P G<br />

9η<br />

Gd<br />

D<br />

D<br />

. (11)<br />

An empirical correlation for the target efficiency for<br />

potential flow around a spherical droplet ( Re D → ∞ ) is<br />

given <strong>by</strong> Langmuir, Pulley (1997)<br />

imp<br />

a ⎟ ⎛ ψ ⎞<br />

η = ⎜<br />

⎝ψ<br />

+ ⎠<br />

with a = 0.<br />

5 and b = 2 .<br />

(12)<br />

Diffusion and Interception<br />

b<br />

Within this work, models for diffusion and interception<br />

proposed <strong>by</strong> Jung (1998) are applied.<br />

The total capturing efficiency is assumed to be the sum <strong>of</strong><br />

the efficiencies due to impaction, diffusion and<br />

interception,<br />

η +<br />

= η + η η . (13)<br />

tot imp diff int<br />

There<strong>by</strong>, the number <strong>of</strong> particles captured <strong>by</strong> one droplet<br />

can be expressed as<br />

N<br />

C<br />

Liquid Film Flow<br />

2<br />

d Dπ<br />

N P<br />

= η tot u P − u D Δt<br />

. (14)<br />

4<br />

dVΔt<br />

As Viswanathan (1998) pointed out, accounting for the<br />

liquid film flowing along the walls is necessary to<br />

accurately describe the physical phenomena occurring in a<br />

Venturi scrubber. The film influences the frictional<br />

pressure drop as well as droplet velocity and size<br />

distribution. Following Chengxin (1996) one can model<br />

liquid wall film using integral boundary layer type<br />

equations. With the help <strong>of</strong> boundary layer assumption<br />

and integral method, the three-dimensional Navier-Stokes<br />

equations can be reduced to two-dimensional equations<br />

defined on the wall boundary.<br />

∂h<br />

+ ∇<br />

∂t<br />

( hu<br />

)<br />

∂<br />

∂t<br />

1<br />

ρ<br />

F<br />

F<br />

s<br />

⋅<br />

( τ − τ )<br />

fs<br />

+ ∇<br />

w<br />

s<br />

S<br />

u F =<br />

(15)<br />

ρ<br />

( h )<br />

⋅<br />

F<br />

( hu<br />

u + C)<br />

F<br />

F<br />

h<br />

+ hg<br />

− ∇<br />

ρ<br />

F<br />

s<br />

=<br />

p<br />

F<br />

S<br />

+<br />

ρ<br />

F<br />

(16)<br />

In above equations u denotes the depth averaged film<br />

F<br />

velocity. For the calculation <strong>of</strong> the shear stress terms and<br />

the convection correction tensor C a prescribed velocity<br />

pr<strong>of</strong>ile is used. The film pressure p which is assumed to<br />

F<br />

be constant over the film height depends on the gas<br />

p , the capillary pressure n ⋅ ∇ − p σ<br />

pressure G<br />

and the droplet impact pressure p with<br />

D,<br />

impact<br />

= σ<br />

s

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