Supernovae general Techniques photometric Alps Full-waveform inversion Methods data analysis Geophysical techniques Stars abundances Asteroids general Seismic imaging Frequency domain Non-linear inverse problem Techniques radial velocities Adjoint state method Densité Tomographie Stars atmospheres Problème inverse non-linéaire Seismic waves Simulation Compound regularization Amphipathic helix Imagerie sismique quantitative haute résolution Acceleration of particles Ab initio intensities Solar wind Galaxy evolution Density Computational seismology Protoplanetary disks Lithosphérique ADMM ALPS Inverse theory Planets and satellites formation ASTEROIDS INDIVIDUAL 6 HEBE Controlled source seismology Minor planets Lithospheric Molecular dynamics Stars fundamental parameters Planetary systems 67P/Churyumov-Gerasimenko Methods observational Télésismique Astrophysics - Earth and Planetary Astrophysics Parallel computation Accretion disks Imagerie sismique Waveform inversion Méthodes directes Planet-disk interactions Instabilities Galaxy disk ArfGAP1 Achernar Amortissement Landau Théorie Configuration interaction ASTEROIDE Dynamo Methane Seismic anisotropy Données multicomposantes Algèbre linéaire Multifrontal method Stars activity Collisional relaxation Radiative transfer Asteroid 3D Hydrodynamics Wave propagation Galaxy abundances Approximations de rang-faible Frequency-domain analysis Turbulence Theory Teleseismic Stars late-type Long-range interacting systems Astrophysics - Solar and Stellar Astrophysics Methods numerical Surveys Inversion de formes d'ondes Systèmes linéaires creux Gravitation Local optimization Plasmas Methods statistical Circumstellar environment Magnetohydrodynamics Planets and satellites dynamical evolution and stability Tomography Accretion Taylor-Green Alpes Optimisation locale Dipole moment surface Tomographie multiparamètres Planets and satellites detection