Source functions and absorptions coefficients for polarized radiation in a given ansiotropic radiation field are calculated for a variety of permitted electric dipole transitions in the L–S coupling limit. Collisional, radiative and magnetic mixing of the ground sublevels are all considered. The polarization of the self-consistent, emergent radiation field is computed, using an anisotropic escape probability formalism to treat the radiative transfer. It is found that the radiative mixing can enhance the polarization for transitions with large angular momentum, and degrees of polarization ≲ 10 per cent are obtained for transitions with small angular momentum
International audienceIn the preceding paper (063.110), the master equation for the atomic density m...
We present the theoretical framework and numerical methods we have implemented to solve the problem ...
We predict that interstellar lines possess a few percent linear polarization provided that the optic...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
The contribution to the expected linear polarization of quasar broad emission and absorption lines f...
The contribution to the expected linear polarization of quasar broad emission and absorption lines f...
This paper highlights very recent advances concerning the identification of new mechanisms that intr...
International audienceThe polarization of radiation emitted in spectral lines provides an important ...
International audienceThe polarization of radiation emitted in spectral lines provides an important ...
The long-standing paradox of the linear polarization signal of the Na i D1 line was recently resolve...
International audienceThe polarization of radiation emitted in spectral lines provides an important ...
International audienceIn the preceding paper (063.110), the master equation for the atomic density m...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
International audienceIn the preceding paper (063.110), the master equation for the atomic density m...
We present the theoretical framework and numerical methods we have implemented to solve the problem ...
We predict that interstellar lines possess a few percent linear polarization provided that the optic...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
The contribution to the expected linear polarization of quasar broad emission and absorption lines f...
The contribution to the expected linear polarization of quasar broad emission and absorption lines f...
This paper highlights very recent advances concerning the identification of new mechanisms that intr...
International audienceThe polarization of radiation emitted in spectral lines provides an important ...
International audienceThe polarization of radiation emitted in spectral lines provides an important ...
The long-standing paradox of the linear polarization signal of the Na i D1 line was recently resolve...
International audienceThe polarization of radiation emitted in spectral lines provides an important ...
International audienceIn the preceding paper (063.110), the master equation for the atomic density m...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
In this paper, we derive in a coherent manner, starting from the basic equations of evolution of a q...
International audienceIn the preceding paper (063.110), the master equation for the atomic density m...
We present the theoretical framework and numerical methods we have implemented to solve the problem ...
We predict that interstellar lines possess a few percent linear polarization provided that the optic...