The linearization of radiative transfer with respect to surface properties
in the UV and visible part of the solar spectrum is presented. The proposed
method is a rigorous extension of the radiative perturbation theory with r
espect to surface properties. Given the forward and adjoint intensity field
, analytical expressions are provided for the linearization of any observab
le related to the radiation field with respect to surface properties charac
terized by Minnaert's and Lambertian bidirectional reflection distribution
function. For the considered surface reflection characteristics, we also di
scuss an extension of the reduction approach of Chandrasekhar as an alterna
tive linearization method. The suitability of both approaches for the combi
ned retrieval of trace gas and surface properties from the backscattered su
nlight in the UV and visible part of the spectrum is discussed. The authors
come to the conclusion that the perturbation theory, for this purpose, rep
resents the superior method because of its general applicability to any par
ameter characterizing the optical properties of the atmosphere and the unde
rlying surface. (C) 2001 Elsevier Science Ltd. All rights reserved.