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

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2.3 Inclusion of Moisture<br />

In formulating the moist Euler equations, we retain the coupling of dry air mass to the prognostic<br />

variables, and we retain the conservation equation for dry air (2.7), as opposed to coupling the<br />

variables to the full (moist) air mass and hence introducing source terms in the mass conservation<br />

equation (2.7). Additionally, we define the coordinate with respect to the dry-air mass. Based<br />

on these principles, the vertical coordinate can be written as<br />

η = (pdh − pdht)/µd<br />

(2.11)<br />

where µd represents the mass of the dry air in the column and pdh and pdht represent the<br />

hydrostatic pressure of the dry atmosphere and the hydrostatic pressure at the top of the dry<br />

atmosphere. The coupled variables are defined as<br />

V = µdv, Ω = µd ˙η, Θ = µdθ. (2.12)<br />

With these definitions, the moist Euler equations can be written as<br />

∂tU + (∇ · Vu)η + µdα∂xp + (α/αd)∂ηp∂xφ = FU<br />

∂tV + (∇ · Vv)η + µdα∂yp + (α/αd)∂ηp∂yφ = FV<br />

∂tW + (∇ · Vw)η − g[(α/αd)∂ηp − µd] = FW<br />

∂tΘ + (∇ · Vθ)η = FΘ<br />

with the diagnostic equation for dry inverse density<br />

(2.13)<br />

(2.14)<br />

(2.15)<br />

(2.16)<br />

∂tµd + (∇ · V)η = 0 (2.17)<br />

∂tφ + µ −1<br />

d [(V · ∇φ)η − gW ] = 0 (2.18)<br />

∂tQm + (V · ∇qm)η = FQm<br />

(2.19)<br />

∂ηφ = −αdµd<br />

and the diagnostic relation for the full pressure (vapor plus dry air)<br />

p = p0(Rdθm/p0αd) γ<br />

(2.20)<br />

(2.21)<br />

In these equations, αd is the inverse density of the dry air (1/ρd) and α is the inverse density<br />

taking into account the full parcel density α = αd(1 + qv + qc + qr + qi + ...) −1 where q∗ are<br />

the mixing ratios (mass per mass of dry air) for water vapor, cloud, rain, ice, etc. Additionally,<br />

θm = θ(1 + (Rv/Rd)qv) ≈ θ(1 + 1.61qv), and Qm = µdqm; qm = qv, qc, qi, ... .<br />

2.4 Map Projections, Coriolis and Curvature Terms<br />

The <strong>ARW</strong> solver currently supports three projections to the sphere— the Lambert conformal,<br />

polar stereographic, and Mercator projections. These projections are described in Haltiner and<br />

Williams (1980). These projections, and the <strong>ARW</strong> implementation of the map factors, assume<br />

that the map factor transformations for x are y are identical at a given point; that is, the<br />

7

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