DOIAbstract
Astronomy and Astrophysics, 446, pp. 403-415, http://dx.doi.org./10.1051/0004-6361:20042540International audienc
Astronomy and Astrophysics, 446, pp. 403-415, http://dx.doi.org./10.1051/0004-6361:20042540International audienc
The random walk of magnetic field lines is examined numerically and analytically in the context of re...
We present a general radiative transfer model appropriate to diagnose the small scale and mostly unr...
Cosmic ray (CR) propagation in a turbulent medium is usually considered in the diffusion approximati...
Astronomy and Astrophysics, 446, pp. 403-415, http://dx.doi.org./10.1051/0004-6361:20042540Internati...
Context. The Hanle effect is used to determine weak turbulent magnetic fields in the solar atmosphe...
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 thesis is devoted to improve our knowledge on the theory of polarized line formation in a magne...
This paper considers the effect of a random magnetic field on Zeeman line transfer, assuming that th...
The microturbulent approximation of turbulent motions is widely used in radiative transfer calculati...
We present a general radiative transfer model which allows the Zeeman diagnostics of complex and un...
The microturbulent approximation of turbulent motions is widely used in radiative transfer calculati...
The degree of linear polarization has recently been found to show wide random variations over the so...
Astronomy and Astrophysics, 485, pp. 275-287, http://dx.doi.org./10.1051/0004-6361:20079160Internati...
The random walk of magnetic field lines is examined numerically and analytically in the context of re...
We present a general radiative transfer model appropriate to diagnose the small scale and mostly unr...
Cosmic ray (CR) propagation in a turbulent medium is usually considered in the diffusion approximati...
Astronomy and Astrophysics, 446, pp. 403-415, http://dx.doi.org./10.1051/0004-6361:20042540Internati...
Context. The Hanle effect is used to determine weak turbulent magnetic fields in the solar atmosphe...
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 thesis is devoted to improve our knowledge on the theory of polarized line formation in a magne...
This paper considers the effect of a random magnetic field on Zeeman line transfer, assuming that th...
The microturbulent approximation of turbulent motions is widely used in radiative transfer calculati...
We present a general radiative transfer model which allows the Zeeman diagnostics of complex and un...
The microturbulent approximation of turbulent motions is widely used in radiative transfer calculati...
The degree of linear polarization has recently been found to show wide random variations over the so...
Astronomy and Astrophysics, 485, pp. 275-287, http://dx.doi.org./10.1051/0004-6361:20079160Internati...
The random walk of magnetic field lines is examined numerically and analytically in the context of re...
We present a general radiative transfer model appropriate to diagnose the small scale and mostly unr...
Cosmic ray (CR) propagation in a turbulent medium is usually considered in the diffusion approximati...
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