Accueil > Séminaires d’Astrophysique > 3D imaging of the solar interior

 

3D imaging of the solar interior

Laurent Gizon (Max-Planck-Institut für Sonnensystemforschung, Lindau) — au LATT

Par Francois RINCON - 21/04/2010

 

Séminaires d’Astrophysique

de l’Observatoire Midi-Pyrénées


Séminaire de

Laurent Gizon

(Max-Planck-Institut für Sonnensystemforschung, Lindau)

Jeudi 29 Avril 2010 à 11h

OMP, salle Jules Verne


3D imaging of the solar interior

The cross-covariance of the random wave field recorded at two locations on the solar surface is directly related to the Green’s function between these two points. Cross-covariances are used to make images of the solar interior : 3D maps of flow velocities, internal structure, and the magnetic field. A distinction is made between (i) weak inhomogeneities obtained by solving a linear inverse problem and (ii) strong perturbations, such as surface magnetism, infered using forward numerical modeling techniques. I will show results about solar convection, sunspots, and large-scale flows, which are potentially important to better understand the solar dynamo. I will also discuss observational advances and mention the successful launch of the Solar Dynamics Observatory.

 

 

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Laboratoire Astrophysique de Toulouse - Tarbes (UMR5572)

CNRS (Midi-Pyrénées)

Univ. Paul Sabatier

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