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dc.contributor.authorHurtig, T.
dc.contributor.authorBrenning, N.
dc.contributor.authorGunell, H.
dc.date2013
dc.date.accessioned2016-03-25T11:11:12Z
dc.date.available2016-03-25T11:11:12Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2948
dc.descriptionAmplification of magnetic flux and electric polarization fields caused by a plasma streaming at relativistic velocity in to a magnetic field is discussed. It is shown that the electrostatic polarization field that arises in a plasma beam streaming across magnetic field lines at relativistic velocities will cause an amplification of the magnetic flux. This effect is in complete contrast to the expulsion of the magnetic field from the plasma interior that can be expected in high βK plasmas. The amplification is shown to be caused by the relativistic motion of the space charge layers setting up the polarization field. Three dimensional electromagnetic particle-in-cell simulations that support this theory are presented.
dc.languageeng
dc.titleRelativistic magnetic flux amplification
dc.typeConference
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeElectric polarization
dc.subject.freeElectrostatic polarization
dc.subject.freeFlux amplification
dc.subject.freeMagnetic field line
dc.subject.freeParticle-in-cell simulations
dc.subject.freePlasma streaming
dc.subject.freePolarization field
dc.subject.freeSpace charge layers
dc.subject.freeMagnetic fields
dc.subject.freeMagnetic flux
dc.subject.freeAmplification
dc.source.titleDigest of Technical Papers-IEEE International Pulsed Power Conference
dc.source.page1-6
Orfeo.peerreviewedNo
dc.identifier.doi10.1109/PPC.2013.6627640
dc.identifier.scopus2-s2.0-84888620494


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