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- Q7280375 subject Q7181744.
- Q7280375 subject Q7191009.
- Q7280375 subject Q8811519.
- Q7280375 abstract "Radiative flux, also known as radiative flux density or radiation flux, is the amount of power radiated through a given area, in the form of photons or other elementary particles, typically measured in W/m2. It is used in astronomy to determine the magnitude and spectral class of a star. 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.".
- Q7280375 wikiPageWikiLink Q11388.
- Q7280375 wikiPageWikiLink Q124313.
- Q7280375 wikiPageWikiLink Q1478382.
- Q7280375 wikiPageWikiLink Q15054698.
- Q7280375 wikiPageWikiLink Q179600.
- Q7280375 wikiPageWikiLink Q190096.
- Q7280375 wikiPageWikiLink Q2315892.
- Q7280375 wikiPageWikiLink Q25342.
- Q7280375 wikiPageWikiLink Q3198.
- Q7280375 wikiPageWikiLink Q333.
- Q7280375 wikiPageWikiLink Q6485344.
- Q7280375 wikiPageWikiLink Q7181744.
- Q7280375 wikiPageWikiLink Q7191009.
- Q7280375 wikiPageWikiLink Q7575193.
- Q7280375 wikiPageWikiLink Q830654.
- Q7280375 wikiPageWikiLink Q8811519.
- Q7280375 comment "Radiative flux, also known as radiative flux density or radiation flux, is the amount of power radiated through a given area, in the form of photons or other elementary particles, typically measured in W/m2. It is used in astronomy to determine the magnitude and spectral class of a star.".
- Q7280375 label "Radiative flux".