2.2 Flashcards

1
Q

Specific Intensity Definition

A

Describes radiation field at any
- point r
- time t
- direction ((θ, φ))
Iν(r, t, n̂)

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2
Q

Specific Intensity Formula

A

Iν(r, t, n̂) cosθ dA dt dΩ dν = dEν
- Specific intensity through area dA
- dEν [W Hz-1] amount of radiation energy
- θ angle between surface normal and n̂

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3
Q

Blackbody Radiation Formula

A

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

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4
Q

Radiation Flux Definition

A

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

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5
Q

Radiation Flux Formula

A
  • 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
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6
Q

Integration of a function over all solid angles

A
  • Integration of I over all solid angles:

∫ Iν
= ∫ φ = 0π θ = 0 (Iν(θ, φ) sinθ) dθ dφ

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7
Q

Total Radiation Flux Formula

A

F = ∫ Fν

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8
Q

Energy Density Formula

A
  • 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.
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9
Q

Planck Radiation Energy Density

A
  • 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
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10
Q

Total Energy Density for Planck Radiation

A

U = ∫ Uν dν = a T⁴

  • σ Stefan-Boltzmann constant
  • a = 4σ / c
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11
Q

Stefan-Boltzmann Constant

A

σ = 5.67 * 10-8W/(m²K⁴)

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12
Q

Radiation Pressure Formula

A

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
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13
Q

Radiation pressure for isotropic Planck radiation

A
  • Iν = Bν
  • integration over all directions

Pν = (Bν / c) ∫cos²θ dΩ = 4π / 3 · Bν / c = 1/3 · Uν

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14
Q

Total Radiation Pressure

A

PR = U / 3 = (a / 3) T⁴
- radiation pressure has same units as energy density

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