Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Institut d'Astrophysique Spatiale, CNRS / Universite Paris XI, Orsay, FR
Institut d'Astrophysique Spatiale, France
Institut d'Astrophysique Spatiale, CNRS-Universite Paris Sud, Orsay, France
Institut d'Astrophysique Spatiale, Univ. Paris XI / CNRS, France
Institut d'Astrophysique Spatiale, FR
Institut d'Astrophysique Spatiale, CNRS / UniversitéParis Sud, FR
CNRS, Institut d'Astrophysique Spatiale, Verrieres-le-Buisson, France
CNRS, Laboratoire de Physique Stellaire et Planetaire, Verrieres-le-Buisson, France
Institut d'Astrophysique Spatiale, CNRS - Universite Paris Sud, Orsay, FR
CNRS, Laboratoire de Physique Stellaire et Planetaire, Verrieres-le-Buisson, Essonne, France
Institut d'Astrophysique Spatiale, Univ. Paris XI / CNRS, Bat. 121, F-91405 Orsay cedex, France
Institut d'Astrophysique Spatiale, Université de Paris XI, Bât. 121, 91405 Orsay, France
Institut d'Astrophysique Spatiale d'Astrophysique Spatiale, Univ. Paris XI / CNRS, Bat. 121, F-91405 Orsay Cedex, France
Institut d'Astrophysique Spatiale, Bât. 121, Université Paris XI, 91405 Orsay Cedex, France
Universite Paris, Orsay, France
Paris XI, Univ., Orsay, France
Institut d'Astrophysique Spatiale, Univ. Paris XI / CNRS, Bât. 121, 91405 Orsay Cedex, France of Sciences of the Czech Republic, Ondrejov, Czech Republic
Institut d'Astrophysique Spatiale, CNRS / Université Paris XI UMR 8617, 91405 Orsay Cedex, France
Institut d'Astrophysique Spatiale, Unité Mixte CNRS-Université Paris XI, bât 121, F-91405 Orsay Cedex, France
Institut d'Astrophysique Spatiale, CNRS, Université Paris XI, 91405 Orsay Cedex, France
Inst. d'Astrophysique Spatiale, Verrieres-le-Buisson, France
Institut d'Astrophysique Spatiale, Univ. Paris XI / CNRS, Bât. 121, 91405 Orsay Cedex, France
A center-to-limb analysis of solar MG II lines
A Dynamical Representation of the Solar Chromosphere
A ready-made code for the computation of prominence NLTE models
An Eulerian approach for the computation of oscillation mode visibility
Analysis of the MG II resonance lines in the spectrum of Sirius
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