Mach number dependence of turbulent magnetic field amplification: Solenoidal versus compressive flows

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dc.contributor.authorFederrath, Christoph
dc.contributor.authorChabrier, G.
dc.contributor.authorSchober, Jennifer
dc.contributor.authorBanerjee, Robi
dc.contributor.authorKlessen, R.
dc.contributor.authorSchleicher, Dominik R. G.
dc.date.accessioned2018-11-29T22:53:11Z
dc.date.available2018-11-29T22:53:11Z
dc.date.issued2011
dc.date.updated2018-11-29T07:51:20Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/1885/152405
dc.publisherAmerican Physical Society
dc.sourcePhysical Review Letters
dc.subjectKeywords: Amplification rate; Different-magnetic fields; Divergence free; Saturation levels; Turbulent dynamo; Turbulent magnetic fields; Aerodynamics; Amplification; DC generators; Interactive devices; Mach number; Magnetic fields; Magnetohydrodynamics; Solenoids
dc.titleMach number dependence of turbulent magnetic field amplification: Solenoidal versus compressive flows
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue11
local.bibliographicCitation.lastpage5
local.bibliographicCitation.startpage1
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationChabrier, G., Ecole Normale Superieure de Lyon
local.contributor.affiliationSchober, Jennifer, Universitat Heidelberg
local.contributor.affiliationBanerjee, Robi, Hamburger Sternwarte
local.contributor.affiliationKlessen, R., Zentrum für Astronomie der Universität Heidelberg
local.contributor.affiliationSchleicher, Dominik R. G., Institut fur Astrophysik Georg-August-Universitat
local.contributor.authoremailu5575624@anu.edu.au
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.ariespublicationU3488905xPUB15352
local.identifier.citationvolume107
local.identifier.doi10.1103/PhysRevLett.107.114504
local.identifier.scopusID2-s2.0-80052699456
local.identifier.thomsonID000294783900005
local.identifier.uidSubmittedByU3488905
local.type.statusPublished Version

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