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