Scaling laws in decaying helical hydromagnetic turbulence

DOI10.1002/asna.200510365zbMath1075.85005arXivastro-ph/0209119OpenAlexW2100329508WikidataQ63354233 ScholiaQ63354233MaRDI QIDQ5311906

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Publication date: 29 August 2005

Published in: Astronomische Nachrichten (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0209119

zbMATH Keywords

turbulencemagnetohydrodynamicsearly universe

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Astrophysical cosmology (85A40)

Related Items (4)

Subgrid-scale models of isotropic turbulence need not produce energy backscatter ⋮ Inverse transfer of magnetic helicity in direct numerical simulations of compressible isothermal turbulence: helical transfers ⋮ Helical mode interactions and spectral transfer processes in magnetohydrodynamic turbulence ⋮ Inverse transfer of magnetic helicity in direct numerical simulations of compressible isothermal turbulence: scaling laws

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