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Low Froude Brown dwarfs Epidemic Plasma physics Gravitational effects GPU computing Planets and satellites interiors ISM individual objects Orion B Planets and satellites composition Boosting High performance computing Turbulence Unite and Conquer Sparse matrix Solvation Linear algebra Conservation laws Sharp interface Hyperbolic systems Unite and conquer Cybersecurity Geometric multigrid Radiative transfer Parallel computing Schrödinger equation Stars massive Efficiency Domain decomposition Exascale Accretion disks Calcul haute performance ISM molecules Infrared planetary systems Energy Planets and satellites formation HII regions FFT ISM clouds Magnetohydrodynamics Astrophysics - Solar and Stellar Astrophysics Complex and heterogeneous dynamic system Detection-techniques Accretion Methods data analysis Low-Mach correction Astrophysics - Earth and Planetary Astrophysics CUDA Insider threat Methods statistical Planets and satellites atmospheres Iterative methods Data parallelism Dynamic processes OpenMP Level-Set Well-balanced property Astrometry Astrochemistry Stars formation Water MPI Instrumentation Astrophysics - Astrophysics of Galaxies Methods numerical Compressible two-phase flow Convection Laser Aerodynamics Techniques spectroscopic Big data analysis HPC Adaptive optics-instrumentation Gas dynamics 65Y05 Planets and satellites fundamental parameters Ensemble learning Ghost Fluid method High angular resolution ISM structure Dask Approximate Riemann solver Hydrodynamics High Performance Computing Low Mach correction Supercapacitors Large time steps Supernovae general Linear systems Bagging Planets and satellites gaseous planets Asynchronous communication Godunov-type scheme Electron Big data ISM kinematics and dynamics Two-phase flows Shallow water equations AMITEXFFTP Surface tension Interferometers-planets and satellites