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dc.contributor.authorZiebell, Luiz Fernandopt_BR
dc.contributor.authorYoon, Peter H.pt_BR
dc.contributor.authorWu, C.S.pt_BR
dc.date.accessioned2016-05-14T02:07:58Zpt_BR
dc.date.issued2000pt_BR
dc.identifier.issn1070-664Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/141096pt_BR
dc.description.abstractThe present study constitutes a continuation and improvement of the preceding work by Yoon et al. [J. Geophys. Res. 104, 19801 (1999)]. In the present discussion, an instability of Bernstein waves excited by a beam of energetic electrons is investigated. Special attention is paid to the regime where the ratio of plasma frequency, vpe , to electron gyrofrequency, Ve , is sufficiently higher than unity. An approximate but fairly accurate scheme is introduced to deal with the situation dictated by the condition, vpe 2 /Ve 2e1. The present investigation is motivated by the research in solar radiophysics. However, in this article the emphasis is placed on basic properties of the instability rather than its application.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofPhysics of plasmas. Melville. Vol. 7, no. 11 (Nov. 2000), p. 4720-4728pt_BR
dc.rightsOpen Accessen
dc.subjectFeixes de eletronspt_BR
dc.subjectInstabilidade em plasmaspt_BR
dc.titleMaser-beam instability of Bernstein wavespt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000279124pt_BR
dc.type.originEstrangeiropt_BR


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