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Advanced Research WRF (ARW) Technical Note - MMM - University ...

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If ∆x is less than the user-specified critical length scale lcr, then the length scale used for<br />

calculating both Kh and Kv in (4.6) is lh,v = (∆x∆y∆z) 1/3 (and Kh = Kv = K). If ∆x is<br />

greater than an critical length scale lcr, then the length scale lh = √ ∆x∆y in the calculation<br />

of the horizontal eddy viscosity Kh using (4.6), and lv = ∆z for the calculation of the vertical<br />

eddy viscosity Kv using (4.6).<br />

Additionally, the eddy viscosities for scalar mixing are divided by the turbulent Prandtl<br />

number Pr = 1/3.<br />

Prognostic TKE Closure<br />

For the predicted turbulent kinetic energy option (TKE; see section 4.1.4), the eddy viscosities<br />

are computed using<br />

√<br />

e,<br />

Kh,v = Cklh,v<br />

where e is the turbulent kinetic energy (a prognostic variable in this scheme), Ck is a constant<br />

(typically 0.15 < Ck < 0.25), and l is a length scale.<br />

If the grid spacing ∆x is less than the critical length scale lcr, then<br />

lh,v = min (∆x∆y∆z) 1/3 , 0.76 √ e/N <br />

for N 2 > 0,<br />

lh,v = (∆x∆y∆z) 1/3<br />

for N 2 ≤ 0<br />

(see section 4.1.4 for the calculation of N 2 ). Both the horizontal and vertical eddy viscosities<br />

are multiplied by an inverse turbulent Prandtl number P −1<br />

r = 1 + 2l/(∆x∆y∆z) 1/3 for scalar<br />

mixing. In this case (lcr > ∆x) the horizontal and vertical eddy viscosities are equivalent.<br />

If the grid spacing ∆x is greater than the critical length scale lcr, then lh = √ ∆x∆y for the<br />

calculation of Kh. For calculating Kv,<br />

lv = min ∆z, 0.76 √ e/N <br />

for N 2 > 0,<br />

lv = ∆z for N 2 ≤ 0.<br />

The eddy viscosity used for mixing scalars is divided by a turbulent Prandtl number Pr. The<br />

Prandtl number is 1/3 for the horizontal eddy viscosity Kh, and P −1<br />

r = 1+2l/∆z for the vertical<br />

eddy viscosity Kv.<br />

4.1.4 TKE equation for the 1.5 Order Turbulence Closure<br />

The prognostic equation governing the evolution of the turbulent kinetic energy e is<br />

∂t(µde) + (∇ · Ve)η = µd( shear production + buoyancy + dissipation ). (4.7)<br />

The time integration and the transport terms in (4.7) are integrated in the same manner as for<br />

other scalars (as described in Chapter 3). The right-hand side source and sink terms for e are<br />

given as follows.<br />

Shear Production<br />

The shear production term in (4.7) can be written as<br />

shear production = KhD 2 11 + KhD 2 22 + KvD 2 33 + KhD2 xy<br />

12 + KvD2 xη<br />

13 + KvD2 yη<br />

23 .<br />

27

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