Define the residual-circulation stream function by
This satisfies residual mass conservation identically. Let
The momentum equation is
Differentiate geostrophic balance vertically and hydrostatic pressure meridionally to obtain thermal-wind balance
After a time derivative, the transformed density equation gives
On the other hand, the derivative of momentum gives
Eliminating yields the Eliassen equation for residual circulation
Let
where is the Heaviside step function. Then
so the Eliassen equation for residual circulation is
Take no normal residual flow at and , decay as , and choose the streamfunction constant on the connected rigid boundary to be zero. Thus
The required Fourier series in sine modes is
Define
For each mode, the vertical equation is
The Dirac delta function requires
The solution satisfying the boundary conditions is therefore
where
The momentum equation gives
The jump of supplies an equal positive delta function in , so the singular terms cancel. The regular acceleration is
where
Finally, the transformed density equation gives
These exponentially decaying modes are the balanced mean response to wave-activity deposition at .
Let the wave-forcing layer have vertical scale and meridional scale . In the Eliassen equation for residual circulation, the two restoring terms scale as
Their ratio is controlled by
In the shallow-forcing limit , the vertical derivative term dominates:
After one vertical integration,
The Coriolis force on the residual mean circulation therefore balances most of the wave forcing, and
is small at leading order. The response is primarily an overturning circulation with an associated density tendency.
In the deep-forcing limit , the meridional term dominates:
Now
so the residual circulation is too weak to balance the forcing. The dominant momentum response is direct zonal acceleration,
with a comparatively weak overturning and density response.