Fluid Physics
8.292J/12.330J
Problem Set 4
1. Consider the problem of a two-dimensional (infinitely long) airplane wing traveling in the negative x direction at a speed c through an Euler fluid. In the frame of reference of the airplane, the steady flow around the wind looks like
The
wing has width L and the flow over
its upper surface can be characterized by a speed ut, while under the lower surface it has a speed ub. Since the upper surface
is more curved than the lower surface, ut
> ub. The flow has a uniform density and you may neglect gravity in this problem.
a.) Derive an expression for the lift on the wing, per unit length in the y direction. (Hint: Consider the pressure acting on the lower and upper surfaces of the wing.)
b.) In the limit that the flow speeds ut and ub are not very different from c, show that the lift per unit length is proportional to the circulation around the wing, with circulation defined, as usual,
,
where
is a unit vector along the wing surface.
c.) The oncoming flow is irrotational. What can you deduce about the lift of an airplane wing moving through an Euler fluid?
2.
Much of the
circulation of the ocean is driven by the frictional stress exerted on its
surface by the wind. The essential dynamics can be understood using the
vorticity equation for an incompressible fluid. Including the effect of a
turbulent momentum flux, ,
in the vertical direction, this equation is
|
(1) |
where
is the vorticity. In the ocean, the vorticity
is strongly dominated by its vertical component, and the vertical component of
(1) can be written, to a very good approximation, as
|
(2) |
where
is the vertical component of velocity and
is a unit vector in the vertical direction.
If we approximate the flow of the ocean as steady, then
|
(3) |
and using this, (2) becomes
|
(4) |
Now we are interested in flow relative to the rotating earth. From the point of view of an observer in an inertial reference frame, the vertical component of the vorticity can be written
|
(5) |
where
is the earth-relative velocity (i.e. the
velocity we are interested in),
is the angular velocity of the earth, and
is latitude. The second term in (5) is just
twice the projection of the earth's angular velocity vector onto the local
vertical plane, and over most of the ocean, it is substantially larger in
magnitude than the first term on the right of (5).
Next
we substitute (5) into (4) and linearize the result about a state of rest ( =0), with the result that
|
(6) |
where
a is the radius of the earth, and is the south-to-north earth-relative velocity
component. Finally, for simplicity, we consider a range of latitude that is
small enough that we can neglect the variability of the coefficients of (6)
with latitude. Using the definitions
|
|
|
|
where
is some mean latitude, we can further
approximate (6) as
|
(7) |
Equation (7) says that sources of vorticity owing to stretching and to wind stress at the surface must be balanced by north-south flow, bringing in water with higher or lower rotation rates coming from higher or lower latitude. (Water at rest at the equator has no vertical component of rotation,
You are going to make some deductions using (7) and the incompressible mass conservation equation.
Consider
an idealized rectangular ocean basin of dimensions and depth H, phrased in Cartesian
coordinates x, y and z. The basin is assumed to be in the
Northern Hemisphere, so that both
and
are positive. Take the southern boundary of
the basin to lie along
,
the northern boundary to lie along
,
the western boundary to lie along
,
and the eastern boundary to lie along
.
a.) Assuming that the vertical
velocity, ,
vanishes at both the top and bottom of the ocean, and that the wind stress also
vanishes at the bottom (but not the top!), integrate (7) over the whole depth
of the ocean to find an expression for the depth-averaged south-to-north
velocity,
.
b.) Integrate the mass
continuity equation for an incompressible fluid through the depth of the ocean
to find a differential relation between and the depth-averaged west-to-east velocity
component,
.
c.)
The wind
flow over the
|
|
where
is the wind stress at the ocean surface and
is the amplitude of the wind stress curl.
Using
the result of (a) above, find an expression for .
Now using the result of (b) above, find an expression for
.
Note that the boundary condition on
is that it must vanish at both the
eastern and western boundaries. You will not be able to satisfy both of
these conditions. So find two solutions: one that satisfies
=0 on the eastern boundary, and one that
satisfies
=0 on the western boundary.
d.) The reason that both
boundary conditions on cannot be satisfied is that there exists at
either the western or the eastern boundary a thin boundary layer in which all
of the "return flow" is concentrated and in which some of the
approximations we used break down. The most important approximation is the neglect
of the friction of the ocean flowing along the side boundaries. One effect of
this friction is to change the vorticity of the fluid. Note that the wind
stress in our problem provides a negative definite basin-averaged vorticity
tendency. In the steady state, this will have to be balanced by a source.
Considering qualitatively how the side boundary friction might affect
vorticity, at which boundary (east or west) do you think the return flow is
concentrated? Explain your reasoning,
and sketch what the flow might look like (including the boundary layer).
Extra Credit: The effect of side boundary friction can be modeled by adding a term
|
|
to
the right-hand side of (2), where is a coefficient which you may assume is
constant. This term is negligible in the interior, where the solution we
obtained before is valid. But it dominates the right side of (2) in the thin
boundary layer. By obtaining a solution for the thin boundary layer and
matching this to the interior solution at the outer edge of the boundary layer,
find a solution that satisfies both boundary conditions on
and also satisfies
on the continental side of the boundary layer.