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Magnetic field amplification by small-scale dynamo action: Dependence on turbulence models and Reynolds and Prandtl numbers

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dc.contributor.authorSchober, Jennifer
dc.contributor.authorSchleicher, Dominik
dc.contributor.authorFederrath, Christoph
dc.contributor.authorKlessen, Ralf Stephan
dc.contributor.authorBanerjee, Robi
dc.date.accessioned2018-11-29T22:55:20Z
dc.date.available2018-11-29T22:55:20Z
dc.date.issued2012
dc.date.updated2018-11-29T08:05:48Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn1539-3755
dc.identifier.urihttp://hdl.handle.net/1885/153134
dc.publisherAmerican Physical Society
dc.sourcePhysical Review E-Statistical, Nonlinear and Soft Matter Physics
dc.subjectKeywords: Dynamo action; Eigenvalues; Kolmogorov turbulence; Linear differential equation; Magnetic energies; Magnetic field amplification; Magnetic Prandtl numbers; Magnetic Reynolds number; Quantum mechanical; Reynolds; Time evolutions; Turbulent fluctuation; Tur
dc.titleMagnetic field amplification by small-scale dynamo action: Dependence on turbulence models and Reynolds and Prandtl numbers
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage12
local.bibliographicCitation.startpage1
local.contributor.affiliationSchober, Jennifer, Universitat Heidelberg
local.contributor.affiliationSchleicher, Dominik, Georg-August Universitat Gottingen
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationKlessen, Ralf Stephan, Ruprecht Karls University of Heidelberg
local.contributor.affiliationBanerjee, Robi, Hamburger Sternwarte
local.contributor.authoruidFederrath, Christoph, u5575624
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor020199 - Astronomical and Space Sciences not elsewhere classified
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB14767
local.identifier.citationvolume85
local.identifier.doi10.1103/PhysRevE.85.026303
local.identifier.scopusID2-s2.0-84857597311
local.identifier.thomsonID000299994400003
local.type.statusPublished Version

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