Q-Vector Form of Quasi-geostrophic Omega Equation
A version of the QG-omega
equation can be obtained directly from the Equations of Motion with the
beta-plane approximation (p. 249).
See Bluestein, pp. 350-352 for discussion and derivation.
(1)
where the Q-vector is given
by
(2)
For a given static stability and isobaric level, the Q-vector is proportional to the horizontal shear of the geostrophic wind and the horizontal temperature gradients..
The divergence of the Q-vector can be shown to measure the tendency for the geostrophic wind field to locally increase or decrease thickness (alter the shape of the thickness field). It should be noted that this term includes BOTH the changes in thickness (and heights) associated with the translation of features (embedded in the differential vorticity advection term of the QG omega equation) AND the development of features (embedded in the temperature advection term).
The operation required by
equation (1) is obviously not technically difficult, merely involving
calculation of gradients. However,
expansion of the Divergence of Q term is formidable (involving a rule of the
product from hell).
Most of the "flavor" of the QG forcing can be estimated by consideration of the Divergence of Q term alone. In fact, as Bluestein points out, there is a "Trenberth" version of (1) in which the advection of planetary vorticity and the thermal deformation embedded in the far right hand term are neglected on an order of magnitude basis.

In that case, it is often useful merely to PLOT the Q-vectors at points on a chart (rather than attempting an actual calculation of their magnitudes.).
Task: Write a general rule
relating Divergence of Q and the qualitative nature of the QG-induced omega:
(From blackboard discussions in early February 2005 of Q-vectors, but also from simple interpretation of the equation above):
- omega ~ Q-vector convergence
In short, quasigeostrophic forcing for upward motion occurs, at a given level, in areas of Q-vector convergence