Context.The physical interpretation of scattering line polarization offers a novel diagnostic window for exploring the thermal and magnetic structure of the quiet regions of the solar atmosphere. Aims.We evaluate the impact of isotropic collisions with neutral hydrogen atoms on the scattering polarization signals of the 13 lines of multiplet 42 of Ti
International audienceObservations of the Na I D lines polarization in quiet regions near the solar ...
Aims.This paper presents an analysis of the $Q_{1,2}(6{-}12)$ lines of the Q band of the A$^{2}\Pi$-...
International audienceContext: We present a theoretical review of the effect of impact polarization ...
Context.The physical interpretation of scattering line polarization offers a novel diagnostic window...
International audienceContext: The physical interpretation of scattering line polarization offers a ...
International audienceContext: Rigorous modeling of the Ba II lambda4554 formation is potentially in...
Abstract. The linearly polarized solar spectrum that is produced by coherent scattering processes (a...
Context. The atmosphere of the Sun is permeated by a vast amount of magnetic flux that remains invis...
There is a thin transition region (TR) in the solar atmosphere where the temperature rises from 10,0...
Context. We present a theoretical review of the effect of impact polarization of a hydrogen Hα line ...
International audienceIn recent years, Landi Degl'Innocenti ([CITE], [CITE]) has proposed a model of...
Context. One of the challenging theoretical problems in solar physics is the modeling of polarimetri...
We have developed a new semi-classical method for calculating the depolarization and polarization t...
International audienceAims:In light of recent contradictory observational results concerning the ato...
The first theoretical investigation of the formation of the linearly polarized solar line spectrum ...
International audienceObservations of the Na I D lines polarization in quiet regions near the solar ...
Aims.This paper presents an analysis of the $Q_{1,2}(6{-}12)$ lines of the Q band of the A$^{2}\Pi$-...
International audienceContext: We present a theoretical review of the effect of impact polarization ...
Context.The physical interpretation of scattering line polarization offers a novel diagnostic window...
International audienceContext: The physical interpretation of scattering line polarization offers a ...
International audienceContext: Rigorous modeling of the Ba II lambda4554 formation is potentially in...
Abstract. The linearly polarized solar spectrum that is produced by coherent scattering processes (a...
Context. The atmosphere of the Sun is permeated by a vast amount of magnetic flux that remains invis...
There is a thin transition region (TR) in the solar atmosphere where the temperature rises from 10,0...
Context. We present a theoretical review of the effect of impact polarization of a hydrogen Hα line ...
International audienceIn recent years, Landi Degl'Innocenti ([CITE], [CITE]) has proposed a model of...
Context. One of the challenging theoretical problems in solar physics is the modeling of polarimetri...
We have developed a new semi-classical method for calculating the depolarization and polarization t...
International audienceAims:In light of recent contradictory observational results concerning the ato...
The first theoretical investigation of the formation of the linearly polarized solar line spectrum ...
International audienceObservations of the Na I D lines polarization in quiet regions near the solar ...
Aims.This paper presents an analysis of the $Q_{1,2}(6{-}12)$ lines of the Q band of the A$^{2}\Pi$-...
International audienceContext: We present a theoretical review of the effect of impact polarization ...