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Part IA Michaelmas, Lent, Easter Term

Flux Integrals

Surfaces

A surface SS in 3D is often parameterised by:

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))

Orientation: A surface has two sides. The normal vector n\mathbf{n} points to one side.


Surface Element

For a small patch of surface:

  • Normal vector: n\mathbf{n}
  • Area: dSdS
  • Vector area element: dS=ndSd\mathbf{S} = \mathbf{n}\,dS

Definition of Flux Integral

The flux of vector field F\mathbf{F} through surface SS:

Φ=SFdS=SFndS\Phi = \int_S \mathbf{F} \cdot d\mathbf{S} = \int_S \mathbf{F} \cdot \mathbf{n}\,dS

Surface S with normal vectors n, showing vector field F passing through and the flux integral interpretation

Interpretation: Fn\mathbf{F} \cdot \mathbf{n} is the component of F\mathbf{F} through the surface. Added up over SS, this gives total flux.


Physical Examples

  • Fluid flow: Flux = volume of fluid crossing surface per unit time
  • Electric field: Flux = EdS\int \mathbf{E} \cdot d\mathbf{S} (related to enclosed charge)
  • Heat flux: Rate of heat flow through surface

Computing Flux Integrals

Method 1: Parameterisation

For r(u,v)\mathbf{r}(u, v):

dS=ru×rvdudvd\mathbf{S} = \frac{\partial \mathbf{r}}{\partial u} \times \frac{\partial \mathbf{r}}{\partial v}\,du\,dv

Direction given by right-hand rule for (u,v)(u, v) coordinates.

Method 2: Level Surface

For surface g(x,y,z)=cg(x, y, z) = c:

n=±gg\mathbf{n} = \pm \frac{\nabla g}{|\nabla g|}

Choose sign for correct orientation.

Method 3: Graph

For z=f(x,y)z = f(x, y):

ndS=(fx,fy,1)dxdy\mathbf{n}\,dS = \left(-\frac{\partial f}{\partial x}, -\frac{\partial f}{\partial y}, 1\right)dx\,dy


Example: Flux Through a Hemisphere

Find flux of F=(0,0,z)\mathbf{F} = (0, 0, z) through the hemisphere x2+y2+z2=a2x^2 + y^2 + z^2 = a^2, z0z \geq 0, with outward normal.

On the hemisphere: The unit normal is n^=1a(x,y,z)\hat{\mathbf{n}} = \frac{1}{a}(x, y, z).

Fn^=z2a\mathbf{F} \cdot \hat{\mathbf{n}} = \frac{z^2}{a}

Flux = Sz2adS\int_S \frac{z^2}{a}\,dS

By symmetry, x2=y2=z2\langle x^2 \rangle = \langle y^2 \rangle = \langle z^2 \rangle on the sphere, so z2=a23z^2 = \frac{a^2}{3}.

Surface area = 2πa22\pi a^2.

Flux = a2/3a2πa2=2πa33\frac{a^2/3}{a} \cdot 2\pi a^2 = \frac{2\pi a^3}{3}.


Properties

Orientation: Reversing normal multiplies flux by 1-1.

Closed surfaces: For closed surface SS, by convention the normal points outward.


Vector Area

The vector area of a surface:

S=SdS\mathbf{S} = \int_S d\mathbf{S}

Closed surface: Vector area = 0\mathbf{0}

(Each patch cancels with opposite contribution.)


Example: Flat Surface

Flux of F\mathbf{F} through flat surface SS in plane with normal n\mathbf{n}:

Φ=nSFdS\Phi = \mathbf{n} \cdot \int_S \mathbf{F}\,dS

If F\mathbf{F} is constant: Φ=FnArea\Phi = \mathbf{F} \cdot \mathbf{n} \cdot \text{Area}


Why Flux Matters

  • Gauss’s law: Flux through closed surface relates to enclosed source
  • Fluid dynamics: Conservation laws use flux integrals
  • Heat transfer: Thermal flux through boundaries
  • Electromagnetism: Flux of E\mathbf{E} and B\mathbf{B} through surfaces