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Conference Paper: Simulation of relativistic shocks and associated self-consistent radiation

TitleSimulation of relativistic shocks and associated self-consistent radiation
Authors
Nishikawa, K. I.Niemiec, J.Medvedev, M.Zhang, B.Hardee, P.Mizuno, Y.Nordlund, ÅFrederiksen, J.Sol, H.Pohl, M.Hartmann, D. H.Fishman, G. J.
KeywordsParticle-in-cell method (plasma simulation)
Synchrotron radiation by moving charges
Issue Date2010
Citation
Aip Conference Proceedings, 2010, v. 1279, p. 261-264 How to Cite?
DOI: http://dx.doi.org/10.1063/1.3509279
AbstractWe calculated radiation from electrons propagating in a uniform parallel magnetic field to verify our technique. We also used our new technique to calculate emission from electrons in small simulation systems with three different Lorentz factors and ambient parallel magnetic fields. We obtained spectra which are consistent with those generated by electrons propagating in turbulent magnetic fields, that are generated at an early nonlinear stage of the Weibel instability. © 2010 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/361169
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152

 

DC FieldValueLanguage
dc.contributor.authorNishikawa, K. I.-
dc.contributor.authorNiemiec, J.-
dc.contributor.authorMedvedev, M.-
dc.contributor.authorZhang, B.-
dc.contributor.authorHardee, P.-
dc.contributor.authorMizuno, Y.-
dc.contributor.authorNordlund, Å-
dc.contributor.authorFrederiksen, J.-
dc.contributor.authorSol, H.-
dc.contributor.authorPohl, M.-
dc.contributor.authorHartmann, D. H.-
dc.contributor.authorFishman, G. J.-
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. 261-264-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/361169-
dc.description.abstractWe calculated radiation from electrons propagating in a uniform parallel magnetic field to verify our technique. We also used our new technique to calculate emission from electrons in small simulation systems with three different Lorentz factors and ambient parallel magnetic fields. We obtained spectra which are consistent with those generated by electrons propagating in turbulent magnetic fields, that are generated at an early nonlinear stage of the Weibel instability. © 2010 American Institute of Physics.-
dc.languageeng-
dc.relation.ispartofAip Conference Proceedings-
dc.subjectParticle-in-cell method (plasma simulation)-
dc.subjectSynchrotron radiation by moving charges-
dc.titleSimulation of relativistic shocks and associated self-consistent radiation-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.3509279-
dc.identifier.scopuseid_2-s2.0-78649861741-
dc.identifier.volume1279-
dc.identifier.spage261-
dc.identifier.epage264-
dc.identifier.eissn1551-7616-

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