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Kinetic helicity decay in linearly forced turbulence
Stockholm University, Nordic Institute for Theoretical Physics (Nordita). Stockholm University, Faculty of Science, Department of Astronomy.
2012 (English)In: Astronomical Notes - Astronomische Nachrichten, ISSN 0004-6337, E-ISSN 1521-3994, Vol. 333, no 3, 195-201 p.Article in journal (Refereed) Published
Abstract [en]

The decay of kinetic helicity is studied in numerical models of forced turbulence using either an externally imposed forcing function as an inhomogeneous term in the equations or, alternatively, a term linear in the velocity giving rise to a linear instability. The externally imposed forcing function injects energy at the largest scales, giving rise to a turbulent inertial range with nearly constant energy flux while for linearly forced turbulence the spectral energy is maximum near the dissipation wavenumber. Kinetic helicity is injected once a statistically steady state is reached, but it is found to decay on a turbulent time scale regardless of the nature of the forcing and the value of the Reynolds number

Place, publisher, year, edition, pages
2012. Vol. 333, no 3, 195-201 p.
Keyword [en]
hydrodynamics, stars: interiors, turbulence
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-80735DOI: 10.1002/asna.201211654ISI: 000303313300003OAI: oai:DiVA.org:su-80735DiVA: diva2:558659
Note

AuthorCount:2;

Available from: 2012-10-04 Created: 2012-09-27 Last updated: 2017-12-07Bibliographically approved

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Brandenburg, Axel
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