Astronomy and Astrophysics, 453, pp. 1095-1109, http://dx.doi.org./10.1051/0004-6361:20054532International audienc
We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star win...
We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star win...
This paper presents the practical theory that was used to implement the Zeeman effect using Stokes f...
Astronomy and Astrophysics, 453, pp. 1095-1109, http://dx.doi.org./10.1051/0004-6361:20054532Interna...
Context.The Zeeman effect produced by a turbulent magnetic field or a random distribution of flux tu...
Astronomy and Astrophysics, 442, pp. 11-28, http://dx.doi.org./10.1051/0004-6361:20042493Internation...
This paper considers the effect of a random magnetic field on Zeeman line transfer, assuming that th...
We present a general radiative transfer model which allows the Zeeman diagnostics of complex and un...
Astronomy and Astrophysics, 485, pp. 275-287, http://dx.doi.org./10.1051/0004-6361:20079160Internati...
This thesis is devoted to improve our knowledge on the theory of polarized line formation in a magne...
Astronomy and Astrophysics, 446, pp. 403-415, http://dx.doi.org./10.1051/0004-6361:20042540Internati...
Abstract. Stokes parameters measured in the Solar atmosphere are in general time or space averages o...
We present a general radiative transfer model appropriate to diagnose the small scale and mostly unr...
A multiline Bayesian analysis of the Zeeman broadening in the solar atmosphere is presented. A hiera...
Context. The Hanle effect is used to determine weak turbulent magnetic fields in the solar atmosphe...
We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star win...
We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star win...
This paper presents the practical theory that was used to implement the Zeeman effect using Stokes f...
Astronomy and Astrophysics, 453, pp. 1095-1109, http://dx.doi.org./10.1051/0004-6361:20054532Interna...
Context.The Zeeman effect produced by a turbulent magnetic field or a random distribution of flux tu...
Astronomy and Astrophysics, 442, pp. 11-28, http://dx.doi.org./10.1051/0004-6361:20042493Internation...
This paper considers the effect of a random magnetic field on Zeeman line transfer, assuming that th...
We present a general radiative transfer model which allows the Zeeman diagnostics of complex and un...
Astronomy and Astrophysics, 485, pp. 275-287, http://dx.doi.org./10.1051/0004-6361:20079160Internati...
This thesis is devoted to improve our knowledge on the theory of polarized line formation in a magne...
Astronomy and Astrophysics, 446, pp. 403-415, http://dx.doi.org./10.1051/0004-6361:20042540Internati...
Abstract. Stokes parameters measured in the Solar atmosphere are in general time or space averages o...
We present a general radiative transfer model appropriate to diagnose the small scale and mostly unr...
A multiline Bayesian analysis of the Zeeman broadening in the solar atmosphere is presented. A hiera...
Context. The Hanle effect is used to determine weak turbulent magnetic fields in the solar atmosphe...
We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star win...
We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star win...
This paper presents the practical theory that was used to implement the Zeeman effect using Stokes f...
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