omega equation

A diagnostic equation by which the vertical velocity in pressure coordinates (ω = Dp/Dt) may be calculated according to quasigeostrophic theory:

σ

H

2 ω +

f

2

2 ω

p

2

f

∂ p

[

v

g ⋅

H

(

f +

ζ

s ) ] −

H

2

(

v

g ⋅

H

∂ ϕ

∂ p ) {\displaystyle \sigma \nabla _{H}^{2}\omega +f^{2}{\frac {\partial ^{2}\omega }{\partial p^{2}}}=f{\frac {\partial }{\partial p}}\left[\mathbf {v} _{g}\cdot \nabla _{H}\left(f+\zeta _{s}\right)\right]-\nabla _{H}^{2}\left(\mathbf {v} _{g}\cdot \nabla _{H}{\frac {\partial \phi }{\partial p}}\right)} {\displaystyle \sigma \nabla _{H}^{2}\omega +f^{2}{\frac {\partial ^{2}\omega }{\partial p^{2}}}=f{\frac {\partial }{\partial p}}\left[\mathbf {v} _{g}\cdot \nabla _{H}\left(f+\zeta _{s}\right)\right]-\nabla _{H}^{2}\left(\mathbf {v} _{g}\cdot \nabla _{H}{\frac {\partial \phi }{\partial p}}\right)}

for which f is the Coriolis parameter, σ is the static stability, vg is the geostrophic velocity vector, ζg is the geostrophic relative vorticity, φ is the geopotential, ∇H2 is the horizontal Laplacian operator, and H is the horizontal del operator.
The right-hand side of the omega equation can also be expressed in terms of the divergence of the Q vector.
Holton, J. R. 1992. An Introduction to Dynamic Meteorology. 3d edition, Academic Press, . 166–175.