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Path: Thermal/ThermalAnalysis
% Planck's law for a black body.
Also computes the total flux over the range of wavelengths.
Type PlanckL for a demo.
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Form:
PlanckL
[q, lambda, qTotal] = PlanckL( T, lambda )
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Inputs
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T (1,n) Temperature (deg-K)
lambda (n,m) Wavelength vector (micro-meters)
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Outputs
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q (n,m) Black body flux density (watts/m^2-microns)
lambda (n,m) Wavelength vector (micro-meters)
qTotal (n,1) Total flux (watts/m^2)
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References: Thomas, L. C., Heat Transfer, Prentice-Hall, 1992, p. 265
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Common: Graphics/NewFig
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