Astrophysics - Solar and Stellar Astrophysics Galaxy evolution Problème inverse non-linéaire Controlled source seismology Tomographie multiparamètres Solar wind Stars late-type Adjoint state method Radiative transfer Surveys Seismic anisotropy 3D Teleseismic Protoplanetary disks Molecular dynamics Inverse theory Computational seismology Waveform inversion Méthodes directes Galaxy disk 67P/Churyumov-Gerasimenko Planets and satellites formation Taylor-Green Techniques photometric Inversion de formes d'ondes Amortissement Landau Stars fundamental parameters Planetary systems Lithospheric Approximations de rang-faible Techniques radial velocities Galaxy abundances Methods statistical Local optimization Methods numerical Ab initio intensities ALPS Hydrodynamics Simulation Supernovae general ASTEROIDS INDIVIDUAL 6 HEBE Seismic imaging Theory Collisional relaxation Algèbre linéaire Wave propagation Imagerie sismique ADMM Acceleration of particles Planets and satellites dynamical evolution and stability Plasmas Compound regularization Methods data analysis Amphipathic helix Turbulence Gravitation Achernar Stars abundances Planets and satellites detection Binaries close ASTEROIDE Accretion disks Full-waveform inversion Asteroids general Methods observational Instabilities Non-linear inverse problem Astrophysics - Earth and Planetary Astrophysics Tomography Optimisation locale Systèmes linéaires creux Methane Stars activity Théorie Configuration interaction Magnetohydrodynamics Tomographie Alps Long-range interacting systems Dipole moment surface Alpes Stars atmospheres Dynamo Imagerie sismique quantitative haute résolution Planet-disk interactions Données multicomposantes Multifrontal method Circumstellar environment Geophysical techniques Minor planets Frequency domain Télésismique Accretion Frequency-domain analysis Parallel computation Lithosphérique Seismic waves Density Densité Gravitational waves