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