Surfaces
A surface S in 3D is often parameterised by:
r(u,v)=(x(u,v),y(u,v),z(u,v))
Orientation: A surface has two sides. The normal vector n points to one side.
Surface Element
For a small patch of surface:
- Normal vector: n
- Area: dS
- Vector area element: dS=ndS
Definition of Flux Integral
The flux of vector field F through surface S:
Φ=∫SF⋅dS=∫SF⋅ndS

Interpretation: F⋅n is the component of F through the surface. Added up over S, this gives total flux.
Physical Examples
- Fluid flow: Flux = volume of fluid crossing surface per unit time
- Electric field: Flux = ∫E⋅dS (related to enclosed charge)
- Heat flux: Rate of heat flow through surface
Computing Flux Integrals
Method 1: Parameterisation
For r(u,v):
dS=∂u∂r×∂v∂rdudv
Direction given by right-hand rule for (u,v) coordinates.
Method 2: Level Surface
For surface g(x,y,z)=c:
n=±∣∇g∣∇g
Choose sign for correct orientation.
Method 3: Graph
For z=f(x,y):
ndS=(−∂x∂f,−∂y∂f,1)dxdy
Example: Flux Through a Hemisphere
Find flux of F=(0,0,z) through the hemisphere x2+y2+z2=a2, z≥0, with outward normal.
On the hemisphere: The unit normal is n^=a1(x,y,z).
F⋅n^=az2
Flux = ∫Saz2dS
By symmetry, ⟨x2⟩=⟨y2⟩=⟨z2⟩ on the sphere, so z2=3a2.
Surface area = 2πa2.
Flux = aa2/3⋅2πa2=32πa3.
Properties
Orientation: Reversing normal multiplies flux by −1.
Closed surfaces: For closed surface S, by convention the normal points outward.
Vector Area
The vector area of a surface:
S=∫SdS
Closed surface: Vector area = 0
(Each patch cancels with opposite contribution.)
Example: Flat Surface
Flux of F through flat surface S in plane with normal n:
Φ=n⋅∫SFdS
If F is constant: Φ=F⋅n⋅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 and B through surfaces