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Eb
Eb is an EES function that returns the spectral emissive power of a blackbody.
The calling protocol for Eb is:
Eb(T,lambda)
where
T = the temperature (K)
lambda = the wavelength (micron)
Example:
$UnitSystem SI K
$VarInfo E_b units=W/m^2-micron
T=300 [K]
lambda=5 [micron]
E_b=Eb(T,lambda)
{Solution:
E_b=8.176 [W/m^2-micron]
}
Index