“…If the particles constituting the population are of uniform size (assumption that we make throughout this paper for all the particle populations that we deal with), it is known [6] that the spectral scattering phase function λ (θ ) and hence the associated spectral asymmetry factor g λ are unchanged when referring either to a single particle or to a whole population. Concerning the spectral absorption, scattering, and extinction crosssections (respectively, S abs λ , S sca λ , and S ext λ ) produced by a volume V occupied by the particle population, a very straightforward calculation based on the principle of summation of cross-sections yields (11) so that the spectral absorption, scattering, and extinction coefficients (respectively, κ λ , σ λ , and β λ ) produced by the particle population, defined as the related cumulative cross-sections per unit volume, have the following expressions:…”