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arxiv: 1012.1464 · v2 · pith:XOX2GUQInew · submitted 2010-12-07 · 🌌 astro-ph.SR · nlin.CD· physics.ao-ph· physics.flu-dyn· physics.space-ph

Kinetic helicity decay in linearly forced turbulence

classification 🌌 astro-ph.SR nlin.CDphysics.ao-phphysics.flu-dynphysics.space-ph
keywords decayenergyforcedforcinghelicitykineticturbulenceexternally
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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.

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