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