In local thermodynamic equilibrium, matter populations are thermal at the local temperature and the source function is the Planck function, Sν=Bν(T).
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- Blackbody limit of an isothermal atmosphere
- Boltzmann excitation
- Formal solution of the radiative transfer equation
- Free-free absorption
- Grey atmosphere
- Infrared absorber sensitivity kernel
- Limb darkening
- Local radiative equilibrium
- Local thermodynamic equilibrium
- One-layer spectral contrast
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- Radiative transfer source function
- Single-line greenhouse deficit
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