2.2 Flashcards
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
- Integration of I over all solid angles:
Fν = ∫ Iν cosθ dΩ
- Fν = net flux = flux up and flux down = Fν = Fν+ + Fν-
- Fν = 0 for isotropic radiation field inside star or cavity
- Fν = Fν+ and Fν- = 0 outside star or cavity
Integration of a function over all solid angles
- Integration of I 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
- radiation Iν transverses distance c · dt
- fills cylinder c · dt · cosθ · dA
- dEν / (c · dt · cosθ · dA) = (Iν / c) dΩ
→ energy density = integration for all directions:
uν = ∫ (Iν /c) dΩ
- uν = non-isotropic energy density.
Planck Radiation Energy Density
- energy density for isotropic Planck-radiation
Uν = (4π/c) · Bν (T) = (8πh/c³) · (ν³ dν) / (exp(hν/kB T) - 1)
- valid for thermodynamic equilibrium inside star or cavity
- radiation is isotropic
Total Energy Density for Planck Radiation
U = ∫ Uν dν = a T⁴
- σ Stefan-Boltzmann constant
- a = 4σ / c
Stefan-Boltzmann Constant
σ = 5.67 * 10-8W/(m²K⁴)
Radiation Pressure Formula
Pν = (1/c) ∫ Iν cos²θ dΩ
- hν / c = momentum transfer per photon on absorbing material
- dPν = (I / c) dΩ = radiation pressure
- Iν cos θ dΩ = radiation through surface dA
- Iνcos²θ dΩ = momentum component perpendicular to surface dA
Radiation pressure for isotropic Planck radiation
- Iν = Bν
- integration over all directions
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