We develop a radiative transfer model including scattering for Icy moon. We model it as a random medium with rough top and bottom boundaries and a host medium situated beneath. The total scattering and emission consists of three sources: rough boundaries, the volume, and the boundaries and the volume interactions. To account for these sources, we model their respective phase matrices and apply the matrix doubling approach to couple these phase matrices to compute the total emission. The model is then used to explore insights into Icy moon scattering and emission processes. The developed model is readily applied to physical parameters inversion of icy moons.
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Wang et al. (2024) studied this question.
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