23.06.2015 Views

Wind field simulations at Askervein hill - WindSim

Wind field simulations at Askervein hill - WindSim

Wind field simulations at Askervein hill - WindSim

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Considering a neutral ABL, the standard k-ε model is unable to reproduce the right level of<br />

turbulence in the weak shear layer away from the ground. In this region the turbulent viscosity<br />

is overpredicted, (DETERING and ETLING, 1985). The standard model constants have been<br />

modified in an <strong>at</strong>tempt to improve the situ<strong>at</strong>ion. The value of C ε2 , determined from<br />

experiments with decaying grid turbulence, remains unchanged. The diffusion constant σ k ,<br />

close to unity following Reynolds analogy, also remains unchanged. However, the constant<br />

C µ , determined from a shear layer in local equilibrium where it is found to be equal to :<br />

2<br />

⎛ u 1<br />

u 2 ⎞<br />

⎜ ⎟ , has been reduced in accordance with measurements in the ABL (Panofsky, 1977).<br />

⎝ κ ⎠<br />

Finally, the constants C ε1 and C ε2 can be adjusted, guided by the rel<strong>at</strong>ion from a boundary<br />

layer where the logarithmic law is valid :<br />

C<br />

2<br />

κ<br />

= Cε<br />

− C σ<br />

ε1 2<br />

µ ε<br />

Note th<strong>at</strong> κ is the Von Karman constant, set to be 0.4.<br />

The different values of the model constants tested in this work are given in the table below<br />

Constants names C µ C ε1 C ε2 σ k σ ε<br />

Standard values 0.09 1.44 1.92 1.0 1.3<br />

Modified values 0.0324 1.44 1.92 1.0 1.85<br />

2.2.3. Two scale k-ε model<br />

In this model the total turbulence energy, k, is divided equally between the production range<br />

and transfer range, thus k is given by :<br />

k = k p<br />

+ k t<br />

where k p is the turbulent kinetic energy of eddies in the production range and k t is the energy<br />

of eddies in the dissip<strong>at</strong>ion range. For high turbulent Reynolds numbers, the transport<br />

equ<strong>at</strong>ions for the turbulent kinetic energies are:<br />

∂<br />

( ρk<br />

)<br />

∂t<br />

p<br />

∂<br />

+<br />

∂x<br />

i<br />

⎛<br />

⎜ ρk<br />

⎝<br />

p<br />

∂U<br />

∂x<br />

i<br />

ρν<br />

T<br />

−<br />

C<br />

( k )<br />

p<br />

∂k<br />

∂x<br />

p<br />

i<br />

⎞<br />

⎟ = ρ<br />

⎠<br />

( p − ε )<br />

k<br />

p<br />

∂<br />

∂t<br />

( ρk<br />

)<br />

t<br />

∂<br />

+<br />

∂x<br />

i<br />

⎛ ∂U<br />

⎜ ρ<br />

⎝ ∂xi<br />

k<br />

t<br />

ρν<br />

T<br />

−<br />

C<br />

( k )<br />

t<br />

∂k<br />

t<br />

∂x<br />

i<br />

⎞<br />

⎟ = ρ<br />

⎠<br />

( ε − ε )<br />

p<br />

t<br />

wherein; ε p is the transfer r<strong>at</strong>e of turbulent kinetic energy from the production range to the<br />

dissip<strong>at</strong>ion range; ε t is the dissip<strong>at</strong>ion r<strong>at</strong>e; p k is the volumetric production r<strong>at</strong>e of turbulent<br />

kinetic energy; and C(k p ) and C(k t ) are constant coefficients.<br />

The corresponding transport equ<strong>at</strong>ions for the energy transfer r<strong>at</strong>e and the dissip<strong>at</strong>ion r<strong>at</strong>e are<br />

given by :<br />

- 10 -

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!