A method is proposed for the solution of NLTE radiative transfer equations in long cylinders with an external incident radiation that varies with direction. This method is designed principally for the modelling of elongated structures imbedded in the solar corona (loops, prominence threads). The radiative transfer problem under consideration is a 2D one, since the source functions and absorption coefficients vary with both distance to axis and azimuth. The method is based on the general principles of finite-differences and accelerated Λ-iteration. A Fourier series is used for interpolation in azimuth. The method is applied to a line emitted by a two-level atom with complete frequency redistribution. Convergence properties of the method and ...
Exact integral equations are derived describing the source function and radiative flux in a two-dime...
Context: Spectral lines of helium are commonly observed on the Sun. These observations contain impor...
A simplified frequency-integrated radiative transfer equation is solved to study Compton scatterings...
Methods for the solution of non-LTE radiative transfer equations in a cylinder, with external incide...
Aims. Our aim is to improve on previous radiative transfer calculations in illuminated cyl...
This is a review of methods for the solution of non-LTE radiative transfer equations in long cylinde...
Aims. Our aim is to improve on previous radiative transfer calculations in illuminated cylindrical t...
Aims. This paper deals with multidimensional NLTE polarized radiative transfer in the case...
A finite-volume method for radiative transfer in cylindrical enclosures is presented. Angular redist...
In recent years, the interest in radiative heat transfer in cylindrical media has increased primaril...
International audienceThis study is devoted to the examination of scattering of waves by a slab cont...
A multidimensional radiative transfer code is presented, using the short characteristics scheme and...
In this work we present a solution for the radiative conductive transfer equation in cylinder geomet...
. The discretization of the multi--dimensional radiative transfer equation results in a very large l...
Three-dimensional radiative transfer calculations involve extensive amounts of computation. These ca...
Exact integral equations are derived describing the source function and radiative flux in a two-dime...
Context: Spectral lines of helium are commonly observed on the Sun. These observations contain impor...
A simplified frequency-integrated radiative transfer equation is solved to study Compton scatterings...
Methods for the solution of non-LTE radiative transfer equations in a cylinder, with external incide...
Aims. Our aim is to improve on previous radiative transfer calculations in illuminated cyl...
This is a review of methods for the solution of non-LTE radiative transfer equations in long cylinde...
Aims. Our aim is to improve on previous radiative transfer calculations in illuminated cylindrical t...
Aims. This paper deals with multidimensional NLTE polarized radiative transfer in the case...
A finite-volume method for radiative transfer in cylindrical enclosures is presented. Angular redist...
In recent years, the interest in radiative heat transfer in cylindrical media has increased primaril...
International audienceThis study is devoted to the examination of scattering of waves by a slab cont...
A multidimensional radiative transfer code is presented, using the short characteristics scheme and...
In this work we present a solution for the radiative conductive transfer equation in cylinder geomet...
. The discretization of the multi--dimensional radiative transfer equation results in a very large l...
Three-dimensional radiative transfer calculations involve extensive amounts of computation. These ca...
Exact integral equations are derived describing the source function and radiative flux in a two-dime...
Context: Spectral lines of helium are commonly observed on the Sun. These observations contain impor...
A simplified frequency-integrated radiative transfer equation is solved to study Compton scatterings...