No BSD License
20 Oct 2005
20 Oct 2005)
For calculating any exactely any irradiance.
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So, a exact method for calculate any irradiance for any (and many, by a vector)delta wavelength for any wavelenght) by the law of blackbodies functions. For exemple, we compare 3 wavelenght for 3 delta for a vector temperature into 473-5273 K.