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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
326
Nombre de notices
112
Indicateur d'Open Access
86 %
Evolution des dépôts
mots clés
Methods data analysis
GPU computing
CUDA
Planets and satellites gaseous planets
Calcul haute performance
Checkpointing
Hyperbolic systems
Turbulence
High performance computing
Approximate Riemann solver
Big data analysis
Electrochemistry
Hydrodynamics
Astrometry
Radiative transfer
Density functional theory
GPU
Planets and satellites formation
Plasma physics
ISM molecules
Exoplanet atmospheres
Supernovae general
Bagging
ISM structure
Ensemble learning
Planets and satellites atmospheres
Dask
Two-phase flows
HPC
Conservation laws
Parallel algorithms
Astrochemistry
Aerodynamics
Astrophysics - Solar and Stellar Astrophysics
Methods statistical
Dynamic processes
Boosting
ISM individual objects Orion B
Astrophysics - Earth and Planetary Astrophysics
Compressible two-phase flow
Techniques spectroscopic
High Performance Computing
OpenMP
Electron
Cybersecurity
Supercapacitors
Solvation
Unite and conquer
Distributed computing
Complex and heterogeneous dynamic system
AMITEXFFTP
FFT
Big data
Convection
Data parallelism
MPI
Planets and satellites fundamental parameters
Shallow water equations
Parallel computing
Epidemic
Unite and Conquer
ISM kinematics and dynamics
Low-Mach correction
Schrödinger equation
Sparse matrix
Insider threat
Spectral clustering
Stars massive
Asynchronous communication
Gas dynamics
Linear algebra
Astrophysics - Astrophysics of Galaxies
Well-balanced property
Numerical simulation
Surface tension
Domain decomposition
Exascale
Magnetohydrodynamics
Sharp interface
Efficiency
Embedding
Accretion disks
Water
Accretion
Biomarker
Planets and satellites terrestrial planets
ISM clouds
Deep Learning
FPGA
Arnoldi method
Compressible flows
Energy
Planets and satellites interiors
Stars formation
Large time steps
Godunov-type scheme
Methods numerical
Planets and satellites composition
Brown dwarfs
Domain decomposition in space method






