We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D disk configuration. The reliability of three Monte-Carlo and two grid-based codes is tested by comparing their results for a set of well-defined cases which differ for optical depth and viewing angle. For all the configurations, the overall shape of the resulting temperature and spectral energy distribution is well reproduced. The solutions we provide can be used for the verification of other RT codes. We also point out the advantages and disadvantages of the various numerical techniques applied to solve the RT problem
Understanding the properties and evolutionary stage of protoplanetary disks requires to be able to d...
Aims. In this paper we present two efficient implementations of the diffusion approximation to be em...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D disk c...
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D disk c...
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D d...
This is the author accepted manuscript. The final version is available from EDP Sciences via the DOI...
Aims. Solving the continuum radiative transfer equation in high opacity media requires sophisticate...
Radiative transfer is introduced as one of the grand challenge problems in astrophysics due to its k...
A revised and greatly improved version of the 3D continuum radiative transfer code MC3D is presented...
We present a new 3D continuum radiative transfer code, MCFOST, based on a Monte-Carlo method. The r...
We present a new continuum 3D radiative transfer code, MCFOST, based on a Monte-Carlo method. MCFOST...
Radiative Transfer (RT) is considered to be one of the four Grand Challenges in Computational Astrop...
Context. The radiative transport of photons through arbitrary three-dimensional (3D) structures of d...
Higher resolution telescopes as well as 3D numerical simulations will require the development of det...
Understanding the properties and evolutionary stage of protoplanetary disks requires to be able to d...
Aims. In this paper we present two efficient implementations of the diffusion approximation to be em...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D disk c...
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D disk c...
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D d...
This is the author accepted manuscript. The final version is available from EDP Sciences via the DOI...
Aims. Solving the continuum radiative transfer equation in high opacity media requires sophisticate...
Radiative transfer is introduced as one of the grand challenge problems in astrophysics due to its k...
A revised and greatly improved version of the 3D continuum radiative transfer code MC3D is presented...
We present a new 3D continuum radiative transfer code, MCFOST, based on a Monte-Carlo method. The r...
We present a new continuum 3D radiative transfer code, MCFOST, based on a Monte-Carlo method. MCFOST...
Radiative Transfer (RT) is considered to be one of the four Grand Challenges in Computational Astrop...
Context. The radiative transport of photons through arbitrary three-dimensional (3D) structures of d...
Higher resolution telescopes as well as 3D numerical simulations will require the development of det...
Understanding the properties and evolutionary stage of protoplanetary disks requires to be able to d...
Aims. In this paper we present two efficient implementations of the diffusion approximation to be em...
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With ...
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