Linked from

The 17 pages that link to Radiant flux, each with the reason it gives.

• Stefan–Boltzmann lawRelated: The law gives emitted radiant flux per unit surface area.

• TransmittanceRelated: Flux measurements can provide the numerator and denominator of transmittance.

• Luminous efficacyRelated: It supplies the radiometric power compared with visually weighted output.

• RadiometryRelated: It is the power whose distribution across wavelength an SPD describes.

• Solar radiationRelated: It expresses total solar energy flow before dividing by an area.

• CandelaRelated: Photometry converts radiant flux into visually weighted quantities such as candela.

• Bolometric luminosityRelated: It is the measurable energy rate from which stellar luminosity can be inferred.