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   » » Wiki: Radiant Flux
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In , radiant flux or radiant power is the emitted, reflected, transmitted, or received per unit time, and spectral flux or spectral power is the radiant flux per unit or , depending on whether the spectrum is taken as a function of frequency or of wavelength. The SI unit of radiant flux is the (W), one per second (), while that of spectral flux in frequency is the watt per () and that of spectral flux in wavelength is the watt per metre ()—commonly the watt per nanometre ().


Mathematical definitions

Radiant flux
Radiant flux, denoted ('e' for "energetic", to avoid confusion with photometric quantities), is defined as \begin{align} \Phi_\mathrm{e} &= \frac{d Q_\mathrm{e}}{d t} \\2pt Q_\mathrm{e} &= \int_{T} \int_{\Sigma} \mathbf{S}\cdot \hat\mathbf{n}\, dA dt \end{align} where The rate of energy flow through the surface fluctuates at the frequency of the radiation, but radiation detectors only respond to the average rate of flow. This is represented by replacing the Poynting vector with the time average of its norm, giving \Phi_\mathrm{e} \approx \int_\Sigma \langle|\mathbf{S}|\rangle \cos \alpha\ dA , where is the time average, and is the angle between and .


Spectral flux
Spectral flux in frequency, denoted Φe, ν, is defined as \Phi_{\mathrm{e},\nu} = \frac{\partial \Phi_\mathrm{e}}{\partial \nu} , where is the frequency.

Spectral flux in wavelength, denoted , is defined as \Phi_{\mathrm{e},\lambda} = \frac{\partial \Phi_\mathrm{e}}{\partial \lambda} , where is the wavelength.


SI radiometry units

See also


Further reading

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