Linked from

The 56 pages that link to Radiative transfer, each with the reason it gives.

• Interstellar extinctionNarrower topic: Extinction is one part of this broader accounting of light moving through interstellar material.

• Solid angleNarrower topic: Its equations integrate radiation over directions, each weighted by solid angle.

• Exoplanet atmosphereNarrower topic: This framework connects atmospheric gases and particles to the light measured from an exoplanet.

• IlluminanceNarrower topic: It provides a broader framework for light transport that produces surface illuminance.

• OpacityNarrower topic: Opacity enters its equations as the control on radiation’s interactions with matter.

• Kirchhoff's laws of spectroscopyNarrower topic: It generalizes the simple source-and-gas arrangements into realistic layered media.

• Kubelka–Munk theoryNarrower topic: Kubelka–Munk is a paint-shop simplification of this broader physical theory.

• Poynting–Robertson effectNarrower topic: Absorption and re-emission determine how photon momentum becomes a drag force.

• Radiative zoneNarrower topic: Radiative diffusion is the optically thick limit of this broader process.

• Solar spectrumNarrower topic: It provides the broader framework for modeling light emerging through solar layers.

• Atmospheric absorptionNarrower topic: It combines absorption with emission and scattering to calculate atmospheric radiation.

• Radiative equilibriumNarrower topic: Radiative equilibrium is a condition imposed on the energy exchanges that radiative transfer describes.

• Radiation (physics)Narrower topic: It combines the processes that govern radiation traveling through matter.

• Submillimetre astronomyNarrower topic: Interpreting submillimetre signals requires accounting for how dust and gas alter radiation.