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Authordc.contributor.authorGomberoff, L. 
Admission datedc.date.accessioned2019-01-29T15:34:31Z
Available datedc.date.available2019-01-29T15:34:31Z
Publication datedc.date.issued2006
Cita de ítemdc.identifier.citationJournal of Geophysical Research: Space Physics, Volumen 111, Issue 12, 2006
Identifierdc.identifier.issn21699402
Identifierdc.identifier.other10.1029/2006JA012053
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/161656
Abstractdc.description.abstractWe consider a fast solar wind-type plasma consisting of electrons, a protons background, and a much more tenuous alpha particle beam. It is shown that such system is unstable against ion acoustic-like waves triggered by finite-amplitude left-hand polarized waves propagating in the direction of the interplanetary magnetic field. The ion acoustic-like waves have similar properties to those found in a plasma with a much denser proton beam (Gomberoff, 2006b). Although the alpha particle beam is much more tenuous than the proton beam, the system is equally able to trigger ion acoustic-like waves. Therefore we believe that this effect should be taken into account in the evolution of the fast solar wind.
Lenguagedc.language.isoen
Publisherdc.publisherBlackwell
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourceJournal of Geophysical Research: Space Physics
Keywordsdc.subjectGeophysics
Keywordsdc.subjectSpace and Planetary Science
Títulodc.titleIon acoustic-like waves triggered by nonlinear circularly polarized waves in the presence of an alpha particle beam
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorlaj
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile