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The 11 pages that link to Radiative transfer equation, each with the reason it gives.

• Radiative transferBroader topic: It combines the processes that govern radiative transfer into a path-by-path balance.

• ConvolutionRelated: Scattering contributions are often modeled by integrating against spatial kernels.

• Optical depthNarrower topic: Optical depth is a path coordinate that simplifies this equation.

• Integral equationRelated: Scattering couples intensities across directions through integral terms.

• RadianceRelated: It tracks radiance as absorption, emission, and scattering alter a beam.

• Absorption coefficientNarrower topic: It places absorption alongside scattering and emission in a full transport model.

• Spectral radianceRelated: It tracks spectral radiance as sources and interactions alter a beam.

• Brightness temperatureRelated: It determines how an observed source’s radiance relates to emitting and intervening material.

• Diffuse reflectanceNarrower topic: It provides a more general account of the transport processes simplified by Kubelka–Munk theory.

• Outgoing longwave radiationNarrower topic: It provides the framework for calculating how atmospheric layers shape radiation reaching space.

• Kubelka–Munk equationNarrower topic: Kubelka–Munk theory approximates radiative transfer with two opposing diffuse fluxes.