The small-scale dynamo: breaking universality at high Mach numbers
From MaRDI portal
Publication:5141425
DOI10.1088/1367-2630/15/2/023017zbMath1451.76054arXiv1301.4371OpenAlexW3102574999WikidataQ62623617 ScholiaQ62623617MaRDI QIDQ5141425
C. Federrath, Jennifer Schober, Wolfram Schmidt, Stefano Bovino, Dominik R. G. Schleicher
Publication date: 18 December 2020
Published in: New Journal of Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1301.4371
Statistical turbulence modeling (76F55) Transition to turbulence (76F06) Fundamentals of turbulence (76F02)
Cites Work
- Unnamed Item
- Helical shell models for MHD
- Growth rate of small-scale dynamo at low magnetic Prandtl numbers
- Dynamo properties of the turbulent velocity field of a saturated dynamo
- Scaling and dissipation in the GOY shell model
- Small-scale dynamo action during the formation of the first stars and galaxies