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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.
Dépôts récents
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Benjamin Fleury, Mathilde Poveda, Yves Benilan, Roméo Veillet, Olivia Vénot, et al.. High-temperature measurements of acetylene VUV absorption cross sections and application to warm exoplanet atmospheres. Astronomy & Astrophysics - A&A, 2025, 693, pp.A82. ⟨10.1051/0004-6361/202451638⟩. ⟨hal-04863985⟩
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Lionel Gelebart, Aldo Marano, Julien Derouillat, Yang Chen, Francesca Boioli, et al.. Extensions du code parallèle AMITEX_FFTP à la mécanique non-locale et aux couplages. CSMA 2019 - 14ème Colloque National en Calcul de Structures, CSMA, LEM3, MSME, Université de Lorraine, Arts et Métiers, CNRS, May 2019, Hyères, France. ⟨hal-04824592⟩
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Benjamin Fleury, Mathilde Poveda, Yves Benilan, Olivia Venot. High Temperature Measurement of Acetylene UV Absorption Cross Section for the Study of Hot Exoplanet Atmospheres. Annual meeting of the French Society of Astronomy and Astrophysics, SF2A, Jun 2023, Strasbourg, France. p.377-380. ⟨hal-04759347⟩
Pour toute question : hal@cea.fr
Nombre de documents
291
Nombre de notices
117
Indicateur d'Open Access
86 %
Evolution des dépôts
mots clés
Complex and heterogeneous dynamic system
Planets and satellites gaseous planets
Interferometers-planets and satellites
Laser
ISM molecules
Approximate Riemann solver
Distributed computing
Dask
Astrochemistry
Adaptive optics-instrumentation
Electron
Planets and satellites composition
Two-phase flows
Godunov-type scheme
Plasma physics
Cybersecurity
Detection-techniques
HPC
Methods statistical
ISM structure
ISM kinematics and dynamics
OpenMP
High angular resolution
Techniques spectroscopic
Instrumentation
Surface tension
Supernovae general
Planets and satellites atmospheres
AMITEXFFTP
Exascale
Magnetohydrodynamics
Aerodynamics
Stars massive
Well-balanced property
Hyperbolic systems
High performance computing
GPU computing
Exoplanet atmospheres
Insider threat
Astrophysics - Astrophysics of Galaxies
Efficiency
FFT
Planets and satellites formation
Ghost Fluid method
Hydrodynamics
Asynchronous communication
Planets and satellites terrestrial planets
Astrophysics - Solar and Stellar Astrophysics
Brown dwarfs
Geometric multigrid
Solvation
Planets and satellites interiors
Accretion disks
Large time steps
Numerical simulation
Unite and Conquer
Methods numerical
Calcul haute performance
Supercapacitors
Big data
Gravitational effects
Data parallelism
Conservation laws
Iterative methods
Domain decomposition
CUDA
Infrared planetary systems
Turbulence
Epidemic
Convection
Stars formation
Water
Energy
HII regions
Accretion
ISM clouds
High Performance Computing
Low-Mach correction
Boosting
Astrometry
Bagging
Shallow water equations
Parallel computing
Compressible two-phase flow
Radiative transfer
Sparse matrix
ISM individual objects Orion B
Schrödinger equation
65Y05
Sharp interface
Dynamic processes
Unite and conquer
Planets and satellites fundamental parameters
Big data analysis
Compressible flows
Methods data analysis
Ensemble learning
Gas dynamics
Astrophysics - Earth and Planetary Astrophysics
MPI