Optical density

Definition: Optical density (or Absorbance) is defined as the (decadic) logarithm of the ratio of incident to transmitted radiant power through a (non-scattering) sample. This quantity is used, e.g., in spectrophotometry to characterize a dissolved chromophore in a non-scattering solution or an optical filter. Absorbance is defined as: A = -log_{10} T = -log_{10}(frac{I_d}{I_0}) where A is the absorbance or optical density, T is the transmittance,I_{d}I_dis the intensity of the transmitted light after the light traveling a pathlength d, andI_{0}I_0is the intensity of the incident light. For a single chromophore, T can be written asT = e^{-mu_a d} = 10^{-epsilon cd}where amu_ais the absorption coefficient, εepsilonis the molar decadic absorption coefficient, c is the concentration of the chromophore. This equation leads toA = epsilon cd = frac{mu_a d}{log_e 10}mu_a = log_e 10 cdot epsilon c = 2.2303 epsilon c$ In fNIRS, optical density (OD) is sometimes used as a synonym for (decadic) attenuation (termed A as well). In this context, attenuation is relevant instead of absorbance since it also includes the effect of light scattering.

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References:

https://doi.org/10.1117%2F1.NPh.8.1.012101

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