Next: Flux Through Cylinders
Up: The flux Integral
Previous: Introduction
Now we need to find
and dS. If the surface S is defined by a
function, z=g(x,y) we can obtain a nice expression for
and dS.
For the normal vector to S at the point (x0,y0,g(x0,y0)) we
can use the normal vector to the tangent plane. Remember that the tangent
plane to g(x,y) at the point (x0,y0) is given by:

or
-gx(x0,y0)x-gy(x0,y0)y+z=c
where c=-gx(x0,y0)x0-gy(x0,y0)y0+g(x0,y0). A
normal vector to the tangent plane is

If we normalize
to get a unit normal vector we get

So the normal vector as a function of
is

The Area of the jth patch can be obtained by finding the vectors
,
which define the edges of the patch (one parallel to the xz-plane and one parallel to the yz-plane????). The area of the patch is
given by
. If we employ the tangent
plane approximation of g(x,y)we can see that
is the vector from (x0,y0,g(x0,y0)) to
or

Similarly
is the vector that points from (x0,y0,g(x0,y0)) to the point
or

Taking the cross product of
and
gives


Finally, the area of the jth patch is

In the limit that
this becomes


When we put these together we get

|  |
(3) |
So we've represented the integral over the surface in terms of an integral
over the region R in the xy-plane over which S sits.
![\begin{displaymath}
\int_{S}\vec{F}\cdot d\vec{A}=\int_{S}\vec{F}\cdot \hat{n}dS...
...x,y)\hat{\imath}-g_{y}(x,y)\hat{j}+\hat{k}\right)
\right] dA
\end{displaymath}](img71.gif)
Where R is the ''shadow'' of S on the xy-plane.
Notes:
Example
- 1.
- Calculate the flux of the vector field
through the upper hemisphere of x2+y2+z2=4 that lies above the rectangle
,
, oriented upward.
Since the surface consists of the upper hemisphere we can solve the equation
of the sphere for
, so the surface is the
graph of a function and we can use
to find
.

The flux integral is

Where R is the rectangle
,
. Now
substitute
to eliminate the z dependence in the
integral. The integral reduces to


Next: Flux Through Cylinders
Up: The flux Integral
Previous: Introduction
Vector Calculus
8/21/1998