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Conference Paper: Magnetic field amplification by relativistic shocks in turbulent medium

TitleMagnetic field amplification by relativistic shocks in turbulent medium
Authors
Mizuno, Y.Pohl, M.Niemiec, J.Zhang, B.Nishikawa, K. I.Hardee, P. E.
KeywordsMagnetohydrodynamics
Relativistic shock
Turbulence
Issue Date2010
Citation
Aip Conference Proceedings, 2010, v. 1279, p. 385-387 How to Cite?
DOI: http://dx.doi.org/10.1063/1.3509320
AbstractWe investigate magnetic field amplification by relativistic turbulence using 2D relativistic magnetohydrodynamic simulations of the interaction between two identical fluids moving with a relativistic velocity and with an inhomogeneous density in the preshock medium. We found that the density inhomogenity distorts the shape of the shock front and leads to turbulent motion in the postshock region. Turbulent motion stretches and deforms the magnetic field lines and creates filamentary structures. The downstream magnetic field is increased significantly by the turbulent motion. © 2010 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/361170
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152

 

DC FieldValueLanguage
dc.contributor.authorMizuno, Y.-
dc.contributor.authorPohl, M.-
dc.contributor.authorNiemiec, J.-
dc.contributor.authorZhang, B.-
dc.contributor.authorNishikawa, K. I.-
dc.contributor.authorHardee, P. E.-
dc.date.accessioned2025-09-16T04:15:06Z-
dc.date.available2025-09-16T04:15:06Z-
dc.date.issued2010-
dc.identifier.citationAip Conference Proceedings, 2010, v. 1279, p. 385-387-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/361170-
dc.description.abstractWe investigate magnetic field amplification by relativistic turbulence using 2D relativistic magnetohydrodynamic simulations of the interaction between two identical fluids moving with a relativistic velocity and with an inhomogeneous density in the preshock medium. We found that the density inhomogenity distorts the shape of the shock front and leads to turbulent motion in the postshock region. Turbulent motion stretches and deforms the magnetic field lines and creates filamentary structures. The downstream magnetic field is increased significantly by the turbulent motion. © 2010 American Institute of Physics.-
dc.languageeng-
dc.relation.ispartofAip Conference Proceedings-
dc.subjectMagnetohydrodynamics-
dc.subjectRelativistic shock-
dc.subjectTurbulence-
dc.titleMagnetic field amplification by relativistic shocks in turbulent medium-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.3509320-
dc.identifier.scopuseid_2-s2.0-78649897737-
dc.identifier.volume1279-
dc.identifier.spage385-
dc.identifier.epage387-
dc.identifier.eissn1551-7616-

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