Results of an extensive validation study of the new radiative transfer code SHARM-3D are described. The code is designed for modeling of unpolarized monochromatic radiative transfer in the visible and near-IR spectra in the laterally uniform atmosphere over an arbitrarily inhomogeneous anisotropic surface. The surface boundary condition is periodic. The algorithm is based on an exact solution derived with the Green's function method. Several parameterizations were introduced into the algorithm to achieve superior performance. As a result, SHARM-3D is 2-3 orders of magnitude faster than the rigorous code SHDOM. It can model radiances over large surface scenes for a number of incidence-view geometries simultaneously. Extensive comparisons aga...
New technologies permit going continuously down into the spatial scale when observing the Earth's at...
This paper describes a new fast line-by-line radiative transfer scheme which computes top of the atm...
The radiative transfer equations for a coupled atmosphere and canopy are solved numerically by an im...
Using our decades-long experience in radiative transfer (RT) code development for Earth science, we ...
International audienceNew high-resolution spectropolarimetric observations of solar prominences requ...
Context.New high-resolution spectropolarimetric observations of solar prominences require improved ...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
Results are summarized for a scientific project devoted to the comparison of four atmospheric radiat...
Based on the Matrix-Operator Method the radiative transfer code STORM (STOkes vector Radiative trans...
A rigorous and modular Monte Carlo radiative transfer model MCRT has been developed to compute radia...
International audienceContext. The radiative transport of photons through arbitrary three-dimensiona...
Context. The radiative transport of photons through arbitrary three-dimensional (3D) structures of d...
Abstract: The solution of radiative transfer boundary problem for the plane-parallel atmos...
Simulation of future satellite images can be applied in order to validate the general mission concep...
Radiative transfer (RT) is a key component for investigating atmospheres of planetary bodies. With t...
New technologies permit going continuously down into the spatial scale when observing the Earth's at...
This paper describes a new fast line-by-line radiative transfer scheme which computes top of the atm...
The radiative transfer equations for a coupled atmosphere and canopy are solved numerically by an im...
Using our decades-long experience in radiative transfer (RT) code development for Earth science, we ...
International audienceNew high-resolution spectropolarimetric observations of solar prominences requ...
Context.New high-resolution spectropolarimetric observations of solar prominences require improved ...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
Results are summarized for a scientific project devoted to the comparison of four atmospheric radiat...
Based on the Matrix-Operator Method the radiative transfer code STORM (STOkes vector Radiative trans...
A rigorous and modular Monte Carlo radiative transfer model MCRT has been developed to compute radia...
International audienceContext. The radiative transport of photons through arbitrary three-dimensiona...
Context. The radiative transport of photons through arbitrary three-dimensional (3D) structures of d...
Abstract: The solution of radiative transfer boundary problem for the plane-parallel atmos...
Simulation of future satellite images can be applied in order to validate the general mission concep...
Radiative transfer (RT) is a key component for investigating atmospheres of planetary bodies. With t...
New technologies permit going continuously down into the spatial scale when observing the Earth's at...
This paper describes a new fast line-by-line radiative transfer scheme which computes top of the atm...
The radiative transfer equations for a coupled atmosphere and canopy are solved numerically by an im...