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Bienvenue sur la collection HAL de la Maison de la Simulation, laboratoire commun au CEA, au CNRS, à l'Université Paris-Saclay et à l'Université Versailles Saint-Quentin. Elle est spécialisée dans le calcul haute performance et les simulations numériques en lien étroit avec les applications physiques, le génie logiciel parallèle, les modèles de programmation, les techniques de visualisation, l'intelligence artificielle et l'informatique quantique.
Nombre de documents
277
Nombre de notices
Indicateur d'Open Access
Evolution des dépôts
mots clés
MPI
Sparse matrix
Ensemble learning
Planets and satellites composition
Aerodynamics
Brown dwarfs
Planets and satellites formation
Gas dynamics
Unite and conquer
Domain decomposition
Insider threat
FFT
Conservation laws
Parallel computing
Schrödinger equation
Water
Compressible flows
Godunov-type scheme
Supernovae general
65Y05
ISM clouds
Infrared planetary systems
Radiative transfer
Linear systems
Astrometry
Bagging
HPC
Gravitational effects
Astrochemistry
AMITEXFFTP
Plasma physics
Well-balanced property
OpenMP
Planets and satellites fundamental parameters
Geometric multigrid
Astrophysics - Earth and Planetary Astrophysics
Dask
Low-Mach correction
Hyperbolic systems
Supercapacitors
Low Froude
Solvation
Convection
High angular resolution
Interferometers-planets and satellites
Astrophysics - Solar and Stellar Astrophysics
Iterative methods
Boosting
Astrophysics - Astrophysics of Galaxies
Electron
Energy
Surface tension
Instrumentation
Accretion
Big data analysis
Stars formation
Sharp interface
Stars massive
High Performance Computing
Hydrodynamics
Big data
Linear algebra
Epidemic
Detection-techniques
HII regions
Methods data analysis
Magnetohydrodynamics
Cybersecurity
Methods numerical
Two-phase flows
Level-Set
High performance computing
Large time steps
ISM molecules
Techniques spectroscopic
Complex and heterogeneous dynamic system
Exascale
Adaptive optics-instrumentation
Unite and Conquer
ISM kinematics and dynamics
Dynamic processes
Planets and satellites gaseous planets
Methods statistical
Planets and satellites interiors
Ghost Fluid method
Compressible two-phase flow
ISM structure
ISM individual objects Orion B
Accretion disks
Data parallelism
GPU computing
Planets and satellites atmospheres
CUDA
Efficiency
Calcul haute performance
Laser
Turbulence
Approximate Riemann solver
Asynchronous communication
Shallow water equations