Modelling supernova-driven turbulence

DOI10.1080/03091929.2019.1634705zbMath1482.76070arXiv1806.01570OpenAlexW3103569200WikidataQ114640056 ScholiaQ114640056MaRDI QIDQ5065696

James F. Hollins, Graeme R. Sarson, Maarit J. Käpylä, Mordecai-Mark Mac Low, Frederick A. Gent

Publication date: 22 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1806.01570

zbMATH Keywords

numerical methodsinstabilitiesartificial diffusivityhigh Mach number shockssupernova-driven turbulence

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Turbulence (76F99) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (3)

Mean fields and fluctuations in compressible magnetohydrodynamic flows ⋮ Introduction ⋮ Spectral characterisation of inertial particle clustering in turbulence

Uses Software

• ZEUS

Cites Work

• Hydromagnetic turbulence in computer simulations
• A survey of several finite difference methods for systems of nonlinear hyperbolic conservation laws
• Large-scale dynamos in turbulent convection with shear
• A 3D MHD model of astrophysical flows: Algorithms, tests and parallelisation
• The formation of a blast wave by a very intense explosion I. Theoretical discussion
• Unnamed Item

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