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Radiative Transfer

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The article was published on 1950-01-01 and is currently open access. It has received 9085 citations till now. The article focuses on the topics: Radiative transfer.

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Radiative transfer through an arbitrarily thick, scattering atmosphere

TL;DR: In this paper, a method based on the spherical harmonics expansion was proposed for solving the equation of radiative transfer in a vertically inhomogeneous planetary atmosphere, which can be used to compute models with an arbitrarily large optical thickness and any scattering phase function.
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Modified spherical harmonics method for solving the radiative transport equation

TL;DR: In this article, a new approach to solving the three-dimensional radiative transport equation with an arbitrary phase function is proposed, based on expanding the angular part of the specific intensity in q-dependent spherical functions for each spatial Fourier component characterized by the vector q.
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An analytic radiative-convective model for planetary atmospheres

TL;DR: In this paper, an analytic one-dimensional radiative-convective model of the thermal structure of planetary atmospheres is presented, which assumes that thermal radiative transfer is gray and can be represented by the twostream approximation.
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The discrete-ordinate method in diffusive regimes

TL;DR: In this article, the authors studied the behavior of the discrete-ordinate method in highly scattering regimes, where the leading behavior of its solution is determined by the solution of a diffusion equation.
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Laboratory measurements of radar backscatter from bare and snow-covered saline ice sheets

TL;DR: In this paper, the authors performed experiments to collect radar backscatter data at Ku (134GHz) and C bands (53GHz) over simulated sea ice at the US Army Cold Regions Research and Engineering Laboratory (CRREL) during the 1990 and 1992 winter seasons.