Use of signed distance fields in Monte Carlo Radiative Transfer
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Updated
Nov 15, 2024 - Fortran
Use of signed distance fields in Monte Carlo Radiative Transfer
A simple method to solve spherical harmonics moment systems, such as the the time-dependent PN and SPN equations, of radiative transfer in 1D-3D geometry.
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Binary systems with circumstellar matter (β Lyrae)
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Подготовка матриц рассеяния для моделирования процесса переноса солнечной радиации в атмосфере
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