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Solar energy radiative intensity

The boundary conditions associated with the radiative transfer equation usually fix the intensity (or the distribution function) for incoming propagation directions. In the context of solar-energy systems, databases contain the incident surface flux density and its spectral distribution n,i/ (rather than the intensity at the boundary) ... [Pg.30]

See other pages where Solar energy radiative intensity is mentioned: [Pg.463]    [Pg.192]    [Pg.33]    [Pg.305]    [Pg.11]    [Pg.103]    [Pg.1]    [Pg.447]    [Pg.276]   
See also in sourсe #XX -- [ Pg.105 ]



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