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dc.contributor.authorSantos, Michel Silva dospt_BR
dc.contributor.authorZiebell, Luiz Fernandopt_BR
dc.contributor.authorGaelzer, Rudipt_BR
dc.date.accessioned2016-06-09T02:08:29Zpt_BR
dc.date.issued2014pt_BR
dc.identifier.issn1070-664Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/142388pt_BR
dc.description.abstractWe investigate the dispersion relation for low frequency electromagnetic waves propagating parallel to the ambient magnetic field, considering that the velocity distributions of ions and electrons can be either bi-Maxwellian of product bi-kappa distributions. The effect of the anisotropy and non-thermal features associated to the product-bi-kappa distributions on the firehose instability are numerically investigated. The general conclusion to be drawn from the results obtained is that the increase in non-thermal features which is consequence of the decrease of the j indexes in the ion distribution contributes to increase the instability in magnitude and wave number range, in comparison with bi- Maxwellian distributions with similar temperature anisotropy, and that the increase of non-thermal features in the electron distribution contributes to the quenching of the instability, which is nevertheless driven by the anisotropy in the ion distribution. Significant differences between results obtained either considering product-bi-kappa distributions or bi-kappa distributions are also reported.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofPhysics of plasmas. Melville. Vol. 21, no. 11 (Nov 2014), 112102, 12 p.pt_BR
dc.rightsOpen Accessen
dc.subjectInstabilidade em plasmaspt_BR
dc.subjectProcessos de transporte em plasmaspt_BR
dc.subjectTemperatura de plasmaspt_BR
dc.subjectPropagacao de ondas eletromagneticas em plasmaspt_BR
dc.subjectRelações de dispersãopt_BR
dc.titleIon firehose instability in plasmas with plasma particles described by product bi-kappa distributionspt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000952104pt_BR
dc.type.originEstrangeiropt_BR


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