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Radiative flux

Radiative flux, also known as radiative flux density or radiation flux (or sometimes power flux density[1]), is the amount of power radiated through a given area, in the form of photons or other elementary particles, typically measured in W/m2.[2] 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.[3] 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.[4] 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. The cooling associated with the divergence of longwave radiation is necessary for creating and sustaining lasting inversion layers close to the surface during polar night. Longwave radiation flux divergence also plays a role in the formation of fog.[5]

SI radiometry units

  1. ^ Standards organizations recommend that radiometric quantities should be denoted with suffix "e" (for "energetic") to avoid confusion with photometric or photon quantities.
  2. ^ a b c d e Alternative symbols sometimes seen: W or E for radiant energy, P or F for radiant flux, I for irradiance, W for radiant exitance.
  3. ^ a b c d e f g Spectral quantities given per unit frequency are denoted with suffix "ν" (Greek letter nu, not to be confused with a letter "v", indicating a photometric quantity.)
  4. ^ a b c d e f g Spectral quantities given per unit wavelength are denoted with suffix "λ".
  5. ^ a b Directional quantities are denoted with suffix "Ω".

See also

References

  1. ^ "Communication Systems/Wireless Transmission". WikiBooks: Communication Systems/Wireless Transmission. Retrieved 2018-12-11.
  2. ^ "Glossary of Meteorology: Radiative Flux". Retrieved 2008-12-24.
  3. ^ Kantha, L.H.; Clayson, Carol (2000). "Small scale processes in geophysical fluid flow". San Diego: Academic Press. {{cite journal}}: Cite journal requires |journal= (help)
  4. ^ Yang, Rongqian; Friedl, Mark A.; Ni, Wenge (July 16, 2001). "Parameterization of shortwave radiation fluxes for nonuniform vegetation canopies in land surface models" (PDF). Journal of Geophysical Research. 106 (D13): 14275–14286. Bibcode:2001JGR...10614275Y. doi:10.1029/2001JD900180.
  5. ^ Hoch, S. W.; Calanca, P.; Philipona, R.; Ohmura, A. (2007). "Year-Round Observation of Longwave Radiative Flux Divergence in Greenland". Journal of Applied Meteorology and Climatology. 46 (9): 1469–1479. Bibcode:2007JApMC..46.1469H. doi:10.1175/JAM2542.1.