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. -------------------------------------------------------------------------- Form: PlanckL [q, lambda, qTotal] = PlanckL( T, lambda ) -------------------------------------------------------------------------- ------ Inputs ------ T (1,n) Temperature (deg-K) lambda (n,m) Wavelength vector (micro-meters) ------- Outputs ------- 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) -------------------------------------------------------------------------- References: Thomas, L. C., Heat Transfer, Prentice-Hall, 1992, p. 265 --------------------------------------------------------------------------
Common: Graphics/NewFig
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