Estimation of absorption and backscattering coefficients from in situ radiometric measurements: theory and validation in case II waters
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Updated: Sep 25, 2026

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
David McKee1, Alex Cunningham, Susanne Craig
1Department of Physics and Applied Physics, University of Strathclyde, 107 Rottenrow, Glasgow, Scotland G4 0NG, United Kingdom. david.mckee@strath.ac.uk
Abstract:
A model that relates the coefficients of absorption (a) and backscattering (b(b)) to diffuse attenuation (K(d)), radiance reflectance (R(L)), and the mean cosine for downward irradiance (mu(d)) is presented. Radiance transfer simulations are used to verify the physical validity of the model for a wide range of water column conditions. Analysis of thee radiance transfer simulations suggest that absorption and backscattering can be estimated with average errors of 1% and 3%, respectively, if the value of mu(d) is known with depth. If the input data set is restricted to variables that can be derived from measurements of upward radiance (L(u)) and downward irradiance (E(d)), it is necessary to use approximate values of mu(d). Examination of three different approximation schemes for mu(d) shows that the average error for estimating a and b(b) increases to approximately 13%. We tested the model by using measurements of L(u) and E(d) collected from case II waters off the west coast of Scotland. The resulting estimates of a and b(b) were compared with independent in situ measurements of these parameters. Average errors for the data set were of the order of 10% for both absorption and backscattering.
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