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