Variable sheet:
--------------------------------------------------------------------------------------- St Input Name Output Unit Comment freq 2.998E13 Hz frequency (Hz) E 1.987E-20 Joule energy (Joule, erg, eV, kcal/mole) v 1000 cm-1 wavenumber (cm-1) 10 lambda m wavelength of light (nm, A, m, cm) 1 m order (unitless) d .01 mm grating constant (cm, mm, m) theta 2.9671739 degrees rotation angle of grating (radians, de 15 Phi degrees monochromator takeoff angle (radians, alpha -12.03283 degrees incidence angle (radians, degrees) beta 17.967174 degrees diffraction angle (radians, degrees) 100 lines lines/mm grating ruling density (lines/mm) AngDisp .00010513 nm-1 Angular dispersion (mm-1, nm-1) LinDisp .00525633 mm/ Linear Dispersion (mm/nm, mm/A) RLD 19.024668 nm/mm Reciprocal linear dispersion (nm/mm, A .5 Fm m Focal length on monochromator (mm, cm, Sg .01902467 m Geometrical spectral bandpass (mm, m, S .01922467 m Spectral bandpass (mm, m, nm, A) Snu 1.9224668 cm-1 Spectral bandpass (cm-1) 1 H cm Slit height (cm, mm, m) 1 W mm Slit width (cm, mm, m) Sd .2 nm diffraction limited resolution (mm, m N 5000 Total number of lines in grating (unit 50 Wg mm aperture (mm, cm, m) FSR .5 m Free spectral range (mm, m, nm, A) omega .00978028 sr acceptance solid angle, steradians Fnumber 8.961263 F-number of monochromator Ap 24.450708 cm2 grating area viewed from entrance slit As .1 cm2 Slit area (cm2, mm2) PhiO 2.3938E-7 watts Radiant power passed by monochromator Blambda .00002573 W/sr/nm/c Source spectral radiance (W/sr/nm/cm2) .5 Top Transmission factor of monochromator .5 emisiv emissivity of blackbody 1200 Tb K Temperature of blackbody (K, C) 1E9 Dstar cm-rootHz Detectivity of detector (cm-rootHz/W) 1 DeltaF Hz electrical bandpass of detector electr 5 Ad mm2 area of detector SNR 1070.537 signal-to-noise ratio for detector lim B 1.871113 W/sr/cm2 Total radiance over all wavelengths peak 2.4141667 m Peak wavelength (nm, A, m, cm) flux 1.205E13 Hz Photon flux, Hz, on detector exponen 1.1983333 exponent of e in Planck's equation LambdaT 12000000 nm K product of lambda and T, nm K D 4.47214E9 detectivity (W-1) nm 10000 nm wavelength in nm shot 1097737.6 Signal-to-photon-noise ratio .1 klam Quantum efficienty of photon detector --------------------------------------------------------------------------------------- Rule sheet: --------------------------------------------------------------------------------------- * d=1/lines * AngDisp = m/(d*cos(beta)) * LinDisp = Fm*AngDisp * RLD=1/LinDisp * Sg=W/LinDisp * S = Sg+Sd * Snu=.1*S/(lambda*lambda) * Sd = lambda/(m*N) * N = Wg/d * theta=beta-Phi * alpha=theta-Phi * m*lambda=2*d*cos(Phi)*sin(theta) * FSR=lambda/(m+1) * omega=Ap/Fm^2 * Ap=Wg^2*cos(alpha) * As=0.01*W*H * PhiO=Blambda*As*omega*Top*Sg*1e6 * Fnumber=Fm/sqrt(4*Ap/pi()) * lambda = 1/v * Blambda = emisiv*1.19111E16*nm^-5/(exp(1.438e7/(nm*Tb))-1) * E = (6.6261E-34)*freq * freq = (2.998E10)/lambda * B=emisiv*1.8047e-12*Tb^4 * peak=2.897e6/Tb * nm=lambda*1e7 * exponent=1.438e7/(nm*Tb) * LambdaT=nm*Tb * Dstar=D*sqrt(Ad*DeltaF) * SNR=PhiO*D * flux=PhiO/E * shot=klam*flux/sqrt(klam*flux) ---------------------------------------------------------------------------------------Download the Dispersive IR model.
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