Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Observatoire de Paris, Section de Meudon, LESIA, 92195 Meudon Cedex, France
Section de Meudon, DASOP, Observatoire de Paris
Paris, Observatoire, Meudon, France
Observatoire de Paris, Section de Meudon, LESIA, 92195 Meudon Principal Cedex, France
LESIA, Observatoire de Paris, Section de Meudon, 92195 Meudon, France
Observatoire de Paris, Section de Meudon, LESIA, 92195 Meudon Principal Cedex, France Observatoire de Paris, Section de Meudon, 92195 Meudon, France
Meudon, Observatoire, Meudon, Hauts-de-Seine, France
Observatoire de Paris, section Meudon, DASOP / LPSH, F-92195 Meudon Principal Cedex, France
Observatoire de Paris, Section de Meudon, F-92195 Meudon Principal Cedex, France
Observatoire de Paris, Section de Meudon, 92195 Meudon Cedex, France
Observatoire de Paris, Section de Meudon, DASOP, 92195 Meudon Principal Cedex, France
Paris, Observatoire, Meudon, Hauts-de-Seine, France
Observatoire de Paris, Section de Meudon, DASOP, F-92195 Meudon Principal Cedex, France
Observatoire de Paris, MP, France
Observatoire de Paris, Laboratoire d'Études Spatiales et d'Instrumentation en Astrophysique
Observatoire de Paris, Section de Meudon, 92195, Meudon, France
Observatoire de Paris, Section d'Astrophysique de Meudon, 92195 Meudon Principal Cedex, France
Observatoire de Paris, Section de Meudon, DASOP-LPSH, UMR 8645, 92195 Meudon Cedex, France
Observatoire de Paris-Meudon, France
Meudon, Observatoire, France
Observatoire de Paris, Section Meudon, 92195 Meudon Principal Cedex, France
LESIA, Observatoire de Paris-Meudon, France
Faculty of Earth Sciences, University of Lyon I, 2 rue Dubois, 69622 Villeurbanne Cedex, France
Observatoire de Paris-Meudon
2D spectroscopy and science with THEMIS
3-D magnetic configurations supporting prominences. II. The lateral feet as a perturbation of a twisted flux-tube
3-D magnetic configurations supporting prominences. III. Evolution of fine structures observed in a filament channel
A large-scale meridional circulation in the convective zone
A non-LTE inversion procedure for chromospheric cloud-like features
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