Aims. We present the implementation of a radiative transfer solver with coherent scattering in the new BIFROS
Context.Higher resolution telescopes as well as 3D numerical simulations will require the developme...
Three-dimensional radiative transfer calculations involve extensive amounts of computation. These ca...
We come back to the analytical solution of the standard transfer problem in a stellar atmosphere. It...
Aims. We present the implementation of a radiative transfer solver with coherent scattering in the n...
Aims. We present the implementation of a radiative transfer solver with coherent scattering in the n...
Aims. We present the implementation of a radiative transfer solver with coherent scattering in the n...
Context. State of the art quantitative spectroscopy utilizes synthetic spectra to extract informatio...
Context. Multi-level non-local thermodynamic equilibrium (NLTE) radiation transfer calculations have...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
Solving the non-LTE radiative transfer problem in stellar atmospheres is computationally demanding. ...
AbstractWe present an algorithm for solving the radiative transfer problem on massively parallel com...
Radiative Transfer (RT) is considered to be one of the four Grand Challenges in Computational Astrop...
Higher resolution telescopes as well as 3D numerical simulations will require the development of det...
. The discretization of the multi--dimensional radiative transfer equation results in a very large l...
Context. Continuum radiative-transfer simulations are necessary for the interpretation of observatio...
Context.Higher resolution telescopes as well as 3D numerical simulations will require the developme...
Three-dimensional radiative transfer calculations involve extensive amounts of computation. These ca...
We come back to the analytical solution of the standard transfer problem in a stellar atmosphere. It...
Aims. We present the implementation of a radiative transfer solver with coherent scattering in the n...
Aims. We present the implementation of a radiative transfer solver with coherent scattering in the n...
Aims. We present the implementation of a radiative transfer solver with coherent scattering in the n...
Context. State of the art quantitative spectroscopy utilizes synthetic spectra to extract informatio...
Context. Multi-level non-local thermodynamic equilibrium (NLTE) radiation transfer calculations have...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
Solving the non-LTE radiative transfer problem in stellar atmospheres is computationally demanding. ...
AbstractWe present an algorithm for solving the radiative transfer problem on massively parallel com...
Radiative Transfer (RT) is considered to be one of the four Grand Challenges in Computational Astrop...
Higher resolution telescopes as well as 3D numerical simulations will require the development of det...
. The discretization of the multi--dimensional radiative transfer equation results in a very large l...
Context. Continuum radiative-transfer simulations are necessary for the interpretation of observatio...
Context.Higher resolution telescopes as well as 3D numerical simulations will require the developme...
Three-dimensional radiative transfer calculations involve extensive amounts of computation. These ca...
We come back to the analytical solution of the standard transfer problem in a stellar atmosphere. It...
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