22. Parametric Surfaces and Surface Integrals

e. Vector Surface Integrals

A vector surface integral is defined as SFdS=SF(R(u,v))Ndudv \iint_S \vec{F}\cdot\,d\vec{S} =\iint_S \vec{F}(\vec R(u,v))\cdot\vec{N}\,du\,dv However, there is one more fine point we need to discuss before computing this type of integral.

2. Orientations

The integral must be independent of the choice of parametrization. Unfortunately, if we do something as simple as reverse the order of the parameters, i.e. uu and vv are interchanged, then the parametrization becomes R(v,u)\vec R(v,u), the tangent vectors eu\vec e_u and ev\vec e_v are interchanged and the normal is now N=ev×eu\vec N=\vec e_v\times\vec e_u which is the negative of what it was. So the dot product F(R(v,u))N\vec{F}(\vec R(v,u))\cdot\vec{N} reverses sign and the integral changes sign. To correct this ambiguity, we need to understand the orientation of the surface. A surface is orientable if it has two sides. For example, the surface of a cylinder has an inside and an outside; a horizontal plane has a top and a bottom. However a mobius strip has only one side; so it is not orientable. For a non-orientable surface, one can compute scalar surface integrals but not vector surface integrals.

PY: Add plots of cylinder and Mobious strip with animations of normal vectors.

An orientation of an orientable surface is a specification of which side of the surface is considered to be the front of the surface. A parametrization R(u,v)\vec R(u,v) of a surface is oriented if the normal vector N=eu×ev\vec N=\vec e_u\times\vec e_v points toward the front of the surface. From now on, when we want to compute a vector surface integral, we need to specify the orientation of the surface and use an oriented parametrization.

In practice, we don't worry about the orientation when we pick the parametrization. If we end up with the normal pointing toward the wrong side of the surface, then we simply reverse the sign of the normal and proceed. We will see this in the example and exercise below.


Orientations of Line Integrals

Line integrals also need to be oriented. The vector line integral ABFds=ABFvdt \int_A^B \vec F\cdot d\vec s=\int_A^B \vec F\cdot \vec v\,dt is understood to be oriented from AA to BB. If we reverse the direction, then the integral will change signs: BAFds=ABFds \int_B^A \vec F\cdot d\vec s=-\int_A^B \vec F\cdot d\vec s The path is usually parametrized by a curve r(t)\vec r(t) for which tt increases from AA to BB, and hence its tangent vector v\vec v points from AA towards BB. However, if we (accidentally) parametrize it with tt increasing from BB to AA, and notice that the tangent vector points backwards, we don't need to go back and reparametrize it, we just reverse the sign of the tangent and proceed. We will see examples of this in the next part of the course on the multivariable calculus Theorems.


The importance of the orientation of a surface becomes clear when we discuss the flux of a vector field through the surface. If V\vec{V} is the velocity field of a fluid then the flux of V\vec{V} through a surface SS is the integral SVdS\displaystyle \iint_S \vec{V}\cdot\,d\vec{S} which measures the amount of fluid which flows through the surface per unit time. If the fluid flows in the direction of the normal, then the flux is positive. If the fluid flows opposite to the normal, then the flux is negative.

Similarly, the orientation of a curve became important when we discussed the circulation of a vector field around a closed curve. If V\vec{V} is the velocity field of a fluid then the circulation of V\vec{V} around a curve CC is the integral CVds\displaystyle \int_C \vec{V}\cdot\,d\vec{s} which measures the amount of fluid which flows around the curve per unit time. If the fluid flows in the direction of the tangent vector, then the circulation is positive. If it flows opposite to the tangent, then the circulation is negative.

Summary: Vector Surface Integrals

  1. Parametrize the surface, R(u,v)\vec R(u,v).
  2. Evaluate the vector field, F\vec F, on the surface to get F(R(u,v))\vec{F}(\vec R(u,v)).
  3. Find the tangent vectors and normal vector N\vec{N}, for the surface.
  4. Verify the normal is oriented properly. If necessary, reverse it.
  5. Compute the dot product, F(R(u,v))N\vec{F}(\vec R(u,v))\cdot\vec{N}.
  6. Evaluate the integral SF(R(u,v))Ndudv\displaystyle \iint_S \vec{F}(\vec R(u,v))\cdot\vec{N}\,du\,dv.

There is no Jacobian involved anywhere in the calculation. In these integrals, N\vec{N} contains terms that serve the same function as a Jacobian. Often, the parameters one uses to parametrize a surface are similar or even identical to those used for cylindrical coordinates (e.g. rr and θ\theta) or spherical coordinates (e.g. ρ\rho and θ\theta or ϕ\phi). It is important to remember that these are parameters for the surface, and we are not actually integrating in cylindrical or spherical coordinates. There is no extra rr or ρ2sinϕ\rho^2\sin\phi.

Compute PFdS\displaystyle \iint_P \vec{F}\cdot\,d\vec{S} where F=xz,yz,z2\vec{F}=\left\langle xz,yz,z^2\right\rangle and the surface is the polar cap (0ϕπ60 \le \phi \le \dfrac{\pi}{6}) of a sphere of radius 22 with the orientation outward from the sphere.

PY: Add plot.

The surface is given by the parametrization: R(θ,ϕ)=2sinϕcosθ,2sinϕsinθ,2cosϕ \vec R(\theta,\phi) =\left\langle 2\sin\phi\cos\theta,2\sin\phi\sin\theta,2\cos\phi\right\rangle (Note: we have chosen the order of the parameters as (θ,ϕ)(\theta,\phi) to emphasize a point later.) Next, we evaluate the vector field on the surface: F(R(θ,ϕ))=4sinϕcosϕcosθ,4sinϕcosϕsinθ,4cos2ϕ \vec{F}(\vec R(\theta,\phi)) =\left\langle 4\sin\phi\cos\phi\cos\theta,4\sin\phi\cos\phi\sin\theta, 4\cos^2\phi\right\rangle We now find the normal vector: N=eθ×eϕ=ı^ȷ^k^2sinϕsinθ2sinϕcosθ02cosϕcosθ2cosϕsinθ2sinϕ=ı^(4sin2ϕcosθ)ȷ^(4sin2ϕsinθ)+k^(4sinϕcosϕsin2θ4sinϕcosϕcos2θ)=4sin2ϕcosθ,4sin2ϕsinθ,4sinϕcosϕ\begin{aligned} \vec{N}=\vec{e}_\theta\times\vec{e}_\phi &=\left| \begin{array}{ccc} \hat{\imath} & \hat{\jmath} & \hat{k} \\ -2\sin\phi\sin\theta & 2\sin\phi\cos\theta & 0 \\ 2\cos\phi\cos\theta & 2\cos\phi\sin\theta & -2\sin\phi \end{array} \right| \\ &=\hat{\imath}(-4\sin^2\phi\cos\theta) -\hat{\jmath}(4\sin^2\phi\sin\theta) \\ &\quad+\hat{k}(-4\sin\phi\cos\phi\sin^2\theta-4\sin\phi\cos\phi\cos^2\theta) \\ &=\left\langle -4\sin^2\phi\cos\theta,-4\sin^2\phi\sin\theta, -4\sin\phi\cos\phi\right\rangle \end{aligned} To check the orientation of the normal, we look at the zz component of the normal. If it is positive, then the normal points up or outward from the sphere. In the upper hemisphere, sinϕ\sin\phi and cosϕ\cos\phi are positive. So the zz component of the normal is negative. This means the normal is inwards, opposite of what we need it to be. So we reverse N\vec{N} and use that value for the remainder of our calculations. Reverse:N=4sin2ϕcosθ,4sin2ϕsinθ,4sinϕcosϕ \text{Reverse:}\qquad\vec{N} =\left\langle 4\sin^2\phi\cos\theta,4\sin^2\phi\sin\theta,4\sin\phi\cos\phi\right\rangle Next, we compute and simplify the dot product: FN=4sinϕcosϕcosθ,4sinϕcosϕsinθ,4cos2ϕ4sin2ϕcosθ,4sin2ϕsinθ,4sinϕcosϕ=16sin3ϕcosϕcos2θ+16sin3ϕcosϕsin2θ+16sinϕcos3ϕ=16sin3ϕcosϕ(cos2θ+sin2θ)+16sinϕcos3ϕ=16sinϕcosϕ(sin2ϕ+cos2ϕ)=16sinϕcosϕ\begin{aligned} \vec{F}\cdot\vec{N} &=\left\langle 4\sin\phi\cos\phi\cos\theta,4\sin\phi\cos\phi\sin\theta,4\cos^2\phi\right\rangle \\ &\quad\cdot\left\langle 4\sin^2\phi\cos\theta,4\sin^2\phi\sin\theta,4\sin\phi\cos\phi\right\rangle \\ &=16\sin^3\phi\cos\phi\cos^2\theta+16\sin^3\phi\cos\phi\sin^2\theta+16\sin\phi\cos^3\phi \\ &=16\sin^3\phi\cos\phi(\cos^2\theta+\sin^2\theta)+16\sin\phi\cos^3\phi \\ &=16\sin\phi\cos\phi(\sin^2\phi+\cos^2\phi) =16\sin\phi\cos\phi \end{aligned} So the integral is PFdS=PF(R(θ,ϕ))Ndθdϕ=0π/602π(16sinϕcosϕ)dθdϕ=2π[8sin2ϕ]0π/6=16πsin2(π6)=4π\begin{aligned} \iint_P \vec{F}\cdot\,d\vec{S} &=\iint_P \vec{F}(\vec R(\theta,\phi))\cdot\vec{N}\,d\theta\,d\phi \\ &=\int_0^{\pi/6}\int_0^{2\pi} (16\sin\phi\cos\phi)\,d\theta\,d\phi \\ &=2\pi\left[8\sin^2\phi\dfrac{}{}\right]_0^{\pi/6} =16\pi\sin^2\left(\dfrac{\pi}{6}\right) =4\pi \end{aligned}

When we parametrized the surface, we could have named it R(ϕ,θ)\vec R(\phi,\theta) with θ\theta and ϕ\phi reversed. Then the normal would have been N=eϕ×eθ=4sin2ϕcosθ,4sin2ϕsinθ,4sinϕcosϕ \vec{N}=\vec{e}_\phi\times\vec{e}_\theta =\left\langle 4\sin^2\phi\cos\theta,4\sin^2\phi\sin\theta,4\sin\phi\cos\phi\right\rangle which is properly oriented and does not need to be flipped. However, in practice, there is no easy way to know in advance which order to use. So use either order and reverse the normal if necessary.

Compute PFdS\displaystyle \iint_P \vec{F}\cdot\,d\vec{S} where F=xz2,yz2,2z3\vec{F}=\left\langle xz^2,yz^2,-2z^3\right\rangle and the surface is the piece of the elliptic paraboloid z=x2+y2z=x^2+y^2 below z=4z=4 orientated with the normal pointing down and out from the paraboloid. The normal vector was found in a previous exercise.

Hint

Don't forget to check the orientation of the normal and reverse it if necessary.

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Answer

PFdS=256π\displaystyle \iint_P \vec{F}\cdot\,d\vec{S}=256\pi

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Solution

From the previous exercise, the parametrization and normal vector are: R(r,θ)=rcosθ,rsinθ,r2N=2r2cosθ,2r2sinθ,r\begin{aligned} \vec R(r,\theta) &=\left\langle r\cos\theta,r\sin\theta,r^2\right\rangle \\ \vec N &=\left\langle -2r^2\cos\theta,-2r^2\sin\theta,r\right\rangle \end{aligned} To check the orientation, notice Nz=r>0N_z=r \gt 0. So N\vec N points up. Further, in the 1st1^\text{st} quadrant, sinθ>0\sin\theta \gt 0 and cosθ>0\cos\theta \gt 0. So Nx<0N_x \lt 0 and Ny<0N_y \lt 0 and so N\vec N points in. Since we need N\vec N to point down and out, we reverse it: Reverse:N=2r2cosθ,2r2sinθ,r \text{Reverse:}\qquad\vec{N} =\left\langle 2r^2\cos\theta,2r^2\sin\theta,-r\right\rangle (Notice we reverse the entire vector.)

On the surface the vector field, F=xz2,yz2,2z3\vec{F}=\left\langle xz^2,yz^2,-2z^3\right\rangle, becomes: F(R(r,θ))=r5cosθ,r5sinθ,2r6 \vec{F}(\vec R(r,\theta)) =\left\langle r^5\cos\theta,r^5\sin\theta,-2r^6\right\rangle The integrand is the dot product: FN=r5cosθ,r5sinθ,2r62r2cosθ,2r2sinθ,r=2r7cos2θ+2r7sin2θ+2r7=4r7\begin{aligned} \vec{F}\cdot\vec{N} &=\left\langle r^5\cos\theta,r^5\sin\theta,-2r^6\right\rangle \\ &\quad\cdot\left\langle 2r^2\cos\theta,2r^2\sin\theta,-r\right\rangle \\ &=2r^7\cos^2\theta+2r^7\sin^2\theta+2r^7 =4r^7 \end{aligned} So the integral is: PFdS=PFNdrdθ=02π024r7drdθ=2π[r82]02=256π\begin{aligned} \iint_P \vec{F}\cdot\,d\vec{S} &=\iint_P \vec{F}\cdot\vec{N}\,dr\,d\theta =\int_0^{2\pi}\int_0^2 4r^7\,dr\,d\theta \\ &=2\pi\left[\dfrac{r^8}{2}\right]_0^2 =256\pi \end{aligned}

Notice that there is NO extra rr in the integrand before the drdθdr\,d\theta because rr and θ\theta are parameters for a surface which just happen to have the same names as the cylindrical coordinates.

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