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Kilotesla plasmoid formation by a trapped relativistic laser beam

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dc.contributor.authorEhret, M.
dc.contributor.authorKochetkov, Y.
dc.contributor.authorBukharskii, N.
dc.contributor.authorStepanishchev, V.
dc.contributor.authorKorneev, P.
dc.contributor.authorКочетков, Юрий Владимирович
dc.contributor.authorБухарский, Николай Дмитриевич
dc.contributor.authorКорнеев, Филипп Александрович
dc.date.accessioned2024-12-25T10:31:54Z
dc.date.available2024-12-25T10:31:54Z
dc.date.issued2022
dc.description.abstractA strong quasistationary magnetic field is generated in hollow targets with curved internal surface under the action of a relativistically intense picosecond laser pulse. Experimental data evidence the formation of quasistationary strongly magnetized plasma structures decaying on a hundred picoseconds timescale, with the magnetic field strength of the kilotesla scale. Numerical simulations unravel the importance of transient processes during the magnetic field generation and suggest the existence of fast and slow regimes of plasmoid evolution depending on the interaction parameters. The proposed setup is suited for perspective highly magnetized plasma application and fundamental studies. © 2022 American Physical Society.
dc.identifier.citationKilotesla plasmoid formation by a trapped relativistic laser beam / Ehret, M. [et al.] // Physical Review E. - 2022. - 106. - № 4. - 10.1103/PhysRevE.106.045211
dc.identifier.doi10.1103/PhysRevE.106.045211
dc.identifier.urihttps://www.doi.org/10.1103/PhysRevE.106.045211
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85141573656&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000880090300002
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/27655
dc.relation.ispartofPhysical Review E
dc.titleKilotesla plasmoid formation by a trapped relativistic laser beam
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue4
oaire.citation.volume106
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