Wind-driven Circulation

The wind-driven circulation of the oceans

The wind-driven circulation of the oceans


M. D.
This flashcard set delves into advanced physics concepts related to wind-driven circulation, suitable for university-level students. It explores key terms like vorticity, Ekman layers, and pressure balances, focusing on the dynamics of wind-driven flows in water bodies. The set is particularly useful for those studying oceanography or atmospheric sciences, as it provides insights into the behavior of waves, velocity, and stress in fluid dynamics. The inclusion of equations and theoretical explanations makes it a valuable resource for understanding complex interactions in wind-driven systems.
Flashcards
35
Students
1
Language
English
Category
Physics
Level
University
Created / Updated
21.07.2018 / 14.08.2018

Flashcards

Argue why geostrophic flow on an f-plane is horizontally non-divergent. The Taylor-Proudman theorem! 

For geostrophic flow on an f-plane we have: 

\(-fv=-\frac{1}{\rho_0 }p_x;\;\; fu=-\frac{1}{\rho_0}p_y\)

since f is per definition uniform on a f-plane, it follows that: \(u_x+v_y=0\)

for continuity we have: \(u_x+v_y+w_z=0\)

It follows that vertical motion is severely restricted, since for example \(w=0\) at the bottom of the ocean. 

A flow that feels the effect of Earth's rotation (e.g. flows in the atmosphere and the ocean that evolve on time scales longer than a day) tend to be very horizontal. Rotation acts to inhibit vertical motion! 

In what horizontal direction tends flow to be on a rotating planet? 

On a rotating planet, flow tends to be along lines of latitude (cf. Sverdrup balance).

The equation for the vertically integrated transport stream function \(\psi \):

\(J(\Psi,f)=\frac{1}{\rho_0}J(p_b,H)+\frac{1}{\rho_0}[\frac{\partial \tau_s^y}{\partial x}-\frac{\partial \tau_s^x}{\partial y}]\) 

or

\(\beta\Psi_x=\frac{1}{\rho_0}J(p_b,H)+\frac{1}{\rho_0}[\frac{\partial \tau_s^y}{\partial x}-\frac{\partial \tau_s^x}{\partial y}]\)

If the total torque on the right hand side is zero, then: 

\(\beta \Psi_x=0\)

from which it follows that \(\Psi \) depends only on latitude and the flow is entirely zonal, i.e. along lines of latitude. Hence the result!

Note that when the ocean has variable bottom topography, then if the flow extends to the bottom of the ocean, and feels the effect of the variable bottom topography, then, in general, the bottom pressure torque isn't zero. Indeed, in an unstratified ocean, the flow tends to follow \(f/H\) contour lines.

 

Density stratification tends to confine the flow near the surface and insulate the flow from the influence of the variable bottom topography. 

Beginning with the linearized density equation:

\(\frac{\partial \rho'}{\partial t}+w\overline{\rho}=0\)

In steady state, this reduces to: 

\(w\overline{\rho}_z=0\)

It follows that in a stratified ocean we must have \(w=0\). This constraint strongly encourages motion in the horizontal. 

Furthermore, the linear vorticity balance is: 

\(\beta v=fw_z+\frac{G(z)}{\rho_0H_E}[\frac{\partial \tau_s^y}{\partial x}-\frac{\partial \tau_s^x}{\partial y}]\)

Since it  is a prediction of linear dynamics that in steady state \(w=0\), it follows that a further prediction of linear dynmics is that:

\(\beta v=\frac{G(z)}{\rho_0H_E}[\frac{\partial \tau_s^y}{\partial x}-\frac{\partial \tau_s^x}{\partial y}]\)

in which case the horizontal flow field has the same vertical structure as \(G(z)\)and hence is confined entirely to the surface mixed layer. The flow is then insulated from the effect of the variable bottom topography and the bottom pressure torque term is zero.