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Radiative flux

amount of power radiated through a given area

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Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionOct 28, 2025
Entity authorityQ7280375
Source-derived summary

Radiative flux, also known as radiative flux density or radiation flux (or sometimes power flux density), is the amount of power radiated through a given area, in the form of photons or other elementary particles, typically expressed in watts per square meter (W/m2). It is used in astronomy to determine the magnitude and spectral class of a star and in meteorology to determine the intensity of the convection in the planetary boundary layer. Radiative flux also acts as a generalization of heat flux, which is equal to the radiative flux when restricted to the infrared spectrum.

When radiative flux is incident on a surface, it is often called irradiance. Flux emitted from a surface may be called radiant exitance or radiant emittance. The ratio of irradiance reflected to the irradiance received by a surface is called albedo.

Geophysics

Shortwave

In geophysics, shortwave flux is a result of specular and diffuse reflection of incident shortwave radiation by the underlying surface. This shortwave radiation, as solar radiation, can have a profound impact on certain biophysical processes of vegetation, such as canopy photosynthesis and land surface energy budgets, by being absorbed into the soil and canopies. As it is the main energy source of most weather phenomena, the solar shortwave radiation is used extensively in numerical weather prediction.

Longwave

Longwave flux is a product of both downwelling infrared energy as well as emission by the underlying surface.

Editorial summary

The public source identifies “Radiative flux” as amount of power radiated through a given area. This brief keeps that definition visible, then builds a research path around Radiative, flux and amount.

Editorial reviewA dependable orientation record for establishing vocabulary, names and a first evidence trail. The current 234-word lead offers orientation but no explicit four-digit date, so chronology should not be assumed. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with Radiative, flux and amount providing the first useful test.
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A short description can identify a subject without explaining its stakes. For “Radiative flux”, the useful work is to connect “amount of power radiated through a given area” to the records capable of establishing context and consequence.

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Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Oct 28, 2025. The linked authority identifier is Q7280375. None of the 0 selected statements returned an explicit reference.

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Source & attribution

This entry incorporates text from Radiative flux” on English Wikipedia. Contributors are listed in the page history. Text is available under the Creative Commons Attribution-ShareAlike 4.0 License. Selected authority identifiers and statements are retrieved from Wikidata under CC0; their references and qualifiers remain part of the verification path.