ConceptComplete

Surface Integrals

Surface integrals extend integration to two-dimensional surfaces in three-dimensional space, computing quantities such as total flux of a vector field through a surface or the mass of a thin shell.


Parametric Surfaces

Definition

A parametric surface is a continuous map r:D→R3\mathbf{r} : D \to \mathbb{R}^3 from a region D⊆R2D \subseteq \mathbb{R}^2 to R3\mathbb{R}^3: r(u,v)=(x(u,v),y(u,v),z(u,v))\mathbf{r}(u, v) = (x(u,v), y(u,v), z(u,v)) The vectors ru=∂r∂u\mathbf{r}_u = \frac{\partial \mathbf{r}}{\partial u} and rv=∂r∂v\mathbf{r}_v = \frac{\partial \mathbf{r}}{\partial v} are tangent to the surface, and the surface element is dS=(ru×rv) du dv,dS=∥ru×rv∥ du dvd\mathbf{S} = (\mathbf{r}_u \times \mathbf{r}_v)\,du\,dv, \quad dS = \|\mathbf{r}_u \times \mathbf{r}_v\|\,du\,dv


Scalar Surface Integrals

Definition

The scalar surface integral of ff over the surface SS parametrized by r(u,v)\mathbf{r}(u,v) is ∬Sf dS=∬Df(r(u,v))∥ru×rv∥ du dv\iint_S f\,dS = \iint_D f(\mathbf{r}(u,v)) \|\mathbf{r}_u \times \mathbf{r}_v\|\,du\,dv For the graph z=g(x,y)z = g(x,y), this becomes ∬Df(x,y,g(x,y))1+gx2+gy2 dA\iint_D f(x, y, g(x,y)) \sqrt{1 + g_x^2 + g_y^2}\,dA.

ExampleSurface area of a sphere

Parametrize the sphere x2+y2+z2=R2x^2 + y^2 + z^2 = R^2 by r(ϕ,θ)=(Rsin⁡ϕcos⁡θ,Rsin⁡ϕsin⁡θ,Rcos⁡ϕ)\mathbf{r}(\phi, \theta) = (R\sin\phi\cos\theta, R\sin\phi\sin\theta, R\cos\phi): ∥rϕ×rθ∥=R2sin⁡ϕ\|\mathbf{r}_\phi \times \mathbf{r}_\theta\| = R^2 \sin\phi A=∫02π∫0πR2sin⁡ϕ dϕ dθ=4πR2A = \int_0^{2\pi}\int_0^{\pi} R^2 \sin\phi\,d\phi\,d\theta = 4\pi R^2


Flux Integrals

Definition

The flux of a vector field F\mathbf{F} through an oriented surface SS is ∬SF⋅dS=∬DF(r(u,v))⋅(ru×rv) du dv\iint_S \mathbf{F} \cdot d\mathbf{S} = \iint_D \mathbf{F}(\mathbf{r}(u,v)) \cdot (\mathbf{r}_u \times \mathbf{r}_v)\,du\,dv The sign depends on the choice of orientation (which side of SS is "outward").

ExampleFlux through a plane

The flux of F=(0,0,1)\mathbf{F} = (0, 0, 1) (upward flow) through the portion of the plane z=1z = 1 over the unit disk DD: ∬SF⋅dS=∬D(0,0,1)⋅(0,0,1) dA=∬DdA=π\iint_S \mathbf{F} \cdot d\mathbf{S} = \iint_D (0, 0, 1) \cdot (0, 0, 1)\,dA = \iint_D dA = \pi

RemarkOrientation of surfaces

A surface is orientable if it has a consistent choice of unit normal n^\hat{\mathbf{n}}. The Mobius strip is the standard example of a non-orientable surface. Flux integrals require orientability; the divergence theorem and Stokes' theorem apply only to orientable surfaces.