Specific Intensity Definition
Describes radiation field at any
- point r
- time t
- direction n̂((θ, φ))
Iν(r, t, n̂)
Specific Intensity Formula
Iν(r, t, n̂) cosθ dA dt dΩ dν = dEν dν
- Specific intensity through area dA
- dEν [W Hz-1] amount of radiation energy
- θ angle between surface normal and n̂
Blackbody Radiation Formula
Bν dν = (2πh/c²) * (ν³ dν) / (exp(hν/kBT) - 1)
Divide both sides by dν and Bν(T) is the specific intensity of blackbody radiation
Radiation Flux Definition
Fν
= total energy of radiation coming from all directions per unit area per unit time
= dEνdν/(dA dt) and integrate over all solid angles
= Intensity flowing through area dA per unit time dt
Radiation Flux Formula
Fν = ∫ Iν cosθ dΩ
Integration of a function over all solid angles
∫ Iν dΩ
= ∫2π φ = 0 ∫π θ = 0 (Iν(θ, φ) sinθ) dθ dφ
Total Radiation Flux Formula
F = ∫ Fν dν
Energy Density Formula
→ energy density = integration for all directions:
uν = ∫ (Iν /c) dΩ
Planck Radiation Energy Density
Uν = (4π/c) · Bν (T) = (8πh/c³) · (ν³ dν) / (exp(hν/kB T) - 1)
Total Energy Density for Planck Radiation
U = ∫ Uν dν = a T⁴
Stefan-Boltzmann Constant
σ = 5.67 * 10-8W/(m²K⁴)
Radiation Pressure Formula
Pν = (1/c) ∫ Iν cos²θ dΩ
Radiation pressure for isotropic Planck radiation
Pν = (Bν / c) ∫cos²θ dΩ = 4π / 3 · Bν / c = 1/3 · Uν
Total Radiation Pressure
PR = U / 3 = (a / 3) T⁴
- radiation pressure has same units as energy density