If one cross-differentiates (2.10) and (2.11) with respect
to y and x and subtracts to eliminate
, the result
is the vorticity equation (linear form)
In general both the Poincare gravity modes and the vortex
modes have vorticity; however the vortex modes are particularly
rich in vorticity as well as slow in temporal evolution.
Following Rossby we approximate the vorticity
using
the geostrophic approximation (4.1) for
,
with f fixed,
however the variability of f is accounted for in
. Moreover
is evaluated using (2.12) rather than the geostrophic approximation.
The resulting quasi-geostrophic vorticity equation is
where
and
the Jacobian of A and B.
Note that (4.3) is only first order in t and hence can admit
only one root for
; the gravity waves have essentially
been ``filtered out'' by use of the quasi-geostrophic relation.
The term
is the restoring term. In order to
gain some appreciation for this and other terms, we may note
that for an inviscid but stratified fluid the potential
absolute vorticity
is conserved following a fluid column of effective thickness
h. This holds for each of the vertical modes if h is taken
as
; for example for the barotropic mode this
gives
. Furthermore, using the geostrophic
approximation for the relative vorticity
for
mode n gives for the potential absolute vorticity of
mode n:
which in the absence of any disturbance reduces to
for the basic state.
Eq. (4.3) is simply the linearized version of
following the fluid at the geostrophic
velocity (4.1). The restoring term
arises if the flow crosses contours of
(i.e., when
is not a function of
).
For example, if the flow is northwards, then f increases
following the fluid; in order that
remain constant,
either
must decrease or
must increase,
or both.
The quantity
when
multiplied by
is the linearized version of the
anomaly of
from
. If one does allow for variations
of D and hence of the
with x, y then a more general
form of the restoring term in (4.3) is
where the vector
is defined by
which is a normalized gradient of potential absolute vorticity for the base state for mode n. For the barotropic mode this reduces to
If D and the
for
are constant then
all
have the common value
whose direction is northwards and whose magnitude is
,
being the geocentric
distance to the water parcel (about 6370 km). Following
almost universal convention we will denote
as
the Rossby parameter.
For barotropic modes on a sloping shelf, the effect of
variable D may dominate over that of f in determining the
magnitude and direction of the effective
parameter
. This can be important in studies of
subinertial quasi-geostrophic shelf waves (Lamb, 1932,
Art. 212; R. O. Reid, J. Mar. Res., 1958; LeBlond and
Mysak, Ch. 10, Vol. 6, The Sea, 1977).