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Collisionless Shocks Driven by Supersonic Plasma Flows with Self-Generated Magnetic Fields

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dc.contributor.authorLi, C. K.
dc.contributor.authorTikhonchuk, V. T.
dc.contributor.authorMoreno, Q.
dc.contributor.authorSio, H.
dc.contributor.authorKorneev, P.
dc.contributor.authorКорнеев, Филипп Александрович
dc.date.accessioned2024-11-21T11:00:15Z
dc.date.available2024-11-21T11:00:15Z
dc.date.issued2019
dc.description.abstract© 2019 American Physical Society.Collisionless shocks are ubiquitous in the Universe as a consequence of supersonic plasma flows sweeping through interstellar and intergalactic media. These shocks are the cause of many observed astrophysical phenomena, but details of shock structure and behavior remain controversial because of the lack of ways to study them experimentally. Laboratory experiments reported here, with astrophysically relevant plasma parameters, demonstrate for the first time the formation of a quasiperpendicular magnetized collisionless shock. In the upstream it is fringed by a filamented turbulent region, a rudiment for a secondary Weibel-driven shock. This turbulent structure is found responsible for electron acceleration to energies exceeding the average energy by two orders of magnitude.
dc.identifier.citationCollisionless Shocks Driven by Supersonic Plasma Flows with Self-Generated Magnetic Fields / Li, C.K. [et al.] // Physical Review Letters. - 2019. - 123. - № 5. - 10.1103/PhysRevLett.123.055002
dc.identifier.doi10.1103/PhysRevLett.123.055002
dc.identifier.urihttps://www.doi.org/10.1103/PhysRevLett.123.055002
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85070266206&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000479002200005
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/18531
dc.relation.ispartofPhysical Review Letters
dc.titleCollisionless Shocks Driven by Supersonic Plasma Flows with Self-Generated Magnetic Fields
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue5
oaire.citation.volume123
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relation.isAuthorOfPublication.latestForDiscoveryc1864031-d8d5-494b-ab4c-9e548b0ef172
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