dc.creatorServidio, S.
dc.creatorCarbone, V.
dc.creatorDmitruk, Pablo Ariel
dc.creatorMatthaeus, W.H.
dc.date.accessioned2018-08-22T17:37:12Z
dc.date.accessioned2018-11-06T13:32:50Z
dc.date.available2018-08-22T17:37:12Z
dc.date.available2018-11-06T13:32:50Z
dc.date.created2018-08-22T17:37:12Z
dc.date.issued2011-12
dc.identifierServidio, S.; Carbone, V.; Dmitruk, Pablo Ariel; Matthaeus, W.H.; Time decorrelation in isotropic magnetohydrodynamic turbulence; Europhysics Letters; Europhysics Letters; 96; 5; 12-2011; 55503-55507
dc.identifier0295-5075
dc.identifierhttp://hdl.handle.net/11336/56609
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1876634
dc.description.abstractTime decorrelation in isotropic incompressible magnetohydrodynamic (MHD) turbulence is studied using three-dimensional numerical simulation. Eulerian and wavenumber-dependent correlation functions are obtained. Scaling with wavenumber separates effects of nonlinear distortion and effects of random sweeping and Alfvénic wave propagation. Results show that the dominant effect is the combined influence of convective sweeping and Alfvénic propagation, both being nonlocal effects on small-scale fluctuations by large-scale fluctuations. This conclusion finds applications in space plasma observation, particle scattering, predictability, and turbulence theory. © Europhysics Letters Association.
dc.languageeng
dc.publisherEurophysics Letters
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1209/0295-5075/96/55003
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectTURBULENCE
dc.subjectMAGNETOHYDRODYNAMICS
dc.subjectSTATISTICS
dc.subjectPLASMAS
dc.titleTime decorrelation in isotropic magnetohydrodynamic turbulence
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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