Stokes' Theorem with a Single Boundary Curve
Let S be a nice surface in R3 with a nice properly
oriented boundary, ∂S, and let F be a nice vector
field on S. Then
∬S∇×F⋅dS=∮∂SF⋅ds
If the boundary of the surface is a single closed curve, then the boundary
must be traversed counterclockwise as seen from the tip of the normal vector
to the surface.
Notice that the relative orientation of the surface and it boundary
is crucial. If you reverse the direction of the normal to the surface,
or if you reverse the direction the boundary curve is traversed (but
not both) then the LHS and RHS of the theorem will not be equal,
they will differ by a minus sign.
The vector field F is nice if it has continuous first
partial derivatives. Similarly, the surface, S, and its boundary,
∂S, are nice if they are defined by parametric functions
with continuous first partial derivatives.
Show Hand
In words, Stokes' theorem says the flux of the curl of a vector field F
over a surface S is equal to the circulation of F around the
boundary curve ∂S.
This makes sense in that ∇×F⋅N
measures the rotation of the stuff around the N-axis. So the left
side is the total rotation on the surface while the right side is the net
rotation around the boundary.
Notice that on the left hand side (LHS) of the theorem, we are integrating
the curl of the vector field, ∇×F
(and not just F). Since
∇×F is a vector field and we are
integrating it over a surface, we need to
dot it into the vector differential of
surface area, dS=Ndudv. Similarly, on
the right hand side (RHS) of the theorem, we are integrating F
(and not its curl). Again, since F is a
vector field and we are integrating it over the boundary
curve, we need to dot it into the
vector differential of arc length,
ds=vdt.
It is recommended that you first compute ∇×F in
rectangular coordinates, and then convert it to the coordinates needed for
the surface integral. Computing ∇×F in other
coordinate systems is beyond the scope of this course.
Recall that Green's theorem related an integral over a region in the plane
to an integral over its boundary curve. Stokes' theorem is a generalization
of Green's theorem to 3 dimensions in which the region in the plane is
deformed into a surface in 3-dimentional space. In fact, Green's theorem
is technically a special case of Stoke's theorem, namely for a surface which
happens to lie in a plane. See the page on the
2D Stokes' Theorem.
Stokes' Theorem is usually applied to a surface whose boundary is a single
closed curve. So that is where we start:
Compute
∬C∇×F⋅dS
for the vector field F=(−yz,xz,z2) over the
cone, C, given by z=x2+y2 for z≤3 oriented down and out.
We use Stokes' Theorem to convert the surface integral over the cone into
a line integral around the boundary of the cone which is a circle.
∬C∇×F⋅dS=∮∂CF⋅ds
The circle may be parametrized by r(θ)=(3cosθ,3sinθ,3).
So its velocity is v=⟨−3sinθ,3cosθ,0⟩.
If we look at this in the first quadrant where sinθ≥0 and
cosθ≥0, then vx≤0 and vy≥0. So v
points counterclockwise, which is backwards! We need v
clockwise. So we reverse v:
Reverse:v=⟨3sinθ,−3cosθ,0⟩
On the curve, the vector field F=(−yz,xz,z2) becomes:
F∣∣∣R(r,θ)=⟨−9sinθ,9cosθ,9⟩
So the line integral is:
∮∂SF⋅ds=∫02πF⋅vdθ=∫02π(−27sin2θ−27cos2θ+0)dθ=−27(2π)=−54π
Check: Surface Integral Directly
To check, we compute the surface integral directly. We start
by computing the curl of F:
∇×F=∣∣∣∣∣∣ı^∂x−yzȷ^∂yxzk^∂zz2∣∣∣∣∣∣=ı^(0−x)−ȷ^(0−−y)+k^(z−−z)=⟨−x,−y,2z⟩
In cylindrical coordinates, the surface is z=r. So a parametrization is:
R(r,θ)=⟨rcosθ,rsinθ,r⟩
On the surface, the curl of F is:
∇×F∣∣∣R(r,θ)=⟨−rcosθ,−rsinθ,2r⟩
The normal is:
N=er×eθ=∣∣∣∣∣∣ı^cosθ−rsinθȷ^sinθrcosθk^10∣∣∣∣∣∣=ı^(0−rcosθ)−ȷ^(0−−rsinθ)+k^(rcos2θ−−rsin2θ)=⟨−rcosθ,−rsinθ,r⟩
This points up and in. (The z-component is positive while the x and
y components are negative in the first quadrant.) So we reverse the normal:
Reverse:N=⟨rcosθ,rsinθ,−r⟩
Finally, we can compute the integral:
∬C∇×F⋅dS=∫02π∫03∇×F∣∣∣R(r,θ)⋅Ndrdθ=∫02π∫03(−r2cos2θ−r2sin2θ−2r2)drdθ=−∫03r2dr∫02π(1+2)dθ=−[3r3]03[3θ]02π=−9(6π)=−54π
Both methods gave the same answer. This checks both computations and also
verifies Stokes' Theorem for this function and surface. Notice how much
easier the line integral was. This will not always be the case.
Use Stokes' Theorem to compute
∬H∇×F⋅dS
for the vector field F=(y,−x,−x2−y2) over the
hemisphere, H, given by z=9−x2−y2 oriented up and out.
By Stokes' Theorem:
∬H∇×F⋅dS=∮∂HF⋅ds
The boundary is the circle of radius 3 in the xy-plane
traversed counterclockwise, which may be parametrized as:
r(θ)=(3cosθ,3sinθ,0)
The velocity is:
v(θ)=⟨−3sinθ,3cosθ,0⟩
which does point counterclockwise.
On the circle, the vector field F=(y,−x,−x2−y2) becomes:
F∣∣∣r(θ)=(3sinθ,−3cosθ,−9cos2θ−9sin2θ)=(3sinθ,−3cosθ,−9)
So the line integral is:
∮∂HF⋅ds=∫02πF⋅vdθ=∫02π(−9sin2θ−9cos2θ+0)dθ=−9(2π)=−18π
We check by computing the surface integral directly. We start
by computing the curl of F:
∇×F=∣∣∣∣∣∣ı^∂xyȷ^∂y−xk^∂z−x2−y2∣∣∣∣∣∣=ı^(−2y)−ȷ^(−2x)+k^(−1−1)=⟨−2y,2x,−2⟩
Since the surface is a hemisphere of radius 3, we parametrize starting
with spherical coordinates and setting ρ=3:
R(ϕ,θ)=⟨3sinϕcosθ,3sinϕsinθ,3cosϕ⟩
On the surface, the curl of F is:
∇×F∣∣∣R(ϕ,θ)=⟨−6sinϕsinθ,6sinϕcosθ,−2⟩
The normal is:
N=eϕ×eθ=∣∣∣∣∣∣ı^3cosϕcosθ−3sinϕsinθȷ^3cosϕsinθ3sinϕcosθk^−3sinϕ0∣∣∣∣∣∣=ı^(−−9sin2ϕcosθ)−ȷ^(−9sin2ϕsinθ)+k^(9sinϕcosϕcos2θ−−9sinϕcosϕsin2θ)=⟨9sin2ϕcosθ,9sin2ϕsinθ,9sinϕcosϕ⟩
This points up and out as desired. Finally, we can compute the integral:
∬H∇×F⋅dS=∫02π∫0π/2∇×F∣∣∣R(r,θ)⋅Ndϕdθ=∫02π∫0π/2(−54sin3ϕsinθcosθ+54sin3ϕsinθcosθ−18sinϕcosϕ)dϕdθ=−18∫02π∫0π/2sinϕcosϕdϕdθ=−18(2π)[2sin2ϕ]0π/2=−18π
Both methods gave the same answer. This checks both computations and also
verifies Stokes' Theorem for this function and surface. Notice how much
easier the line integral was.
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