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Authordc.contributor.authorGomberoff, L. 
Authordc.contributor.authorAstudillo, H. F. 
Admission datedc.date.accessioned2019-01-29T13:47:42Z
Available datedc.date.available2019-01-29T13:47:42Z
Publication datedc.date.issued1998
Cita de ítemdc.identifier.citationPlanetary and Space Science, Volumen 46, Issue 11-12, 1998, Pages 1683-1687
Identifierdc.identifier.issn00320633
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/159788
Abstractdc.description.abstractIt is well known that ion beam-plasma interactions can destabilize right- and left-hand polarized electromagnetic waves. However, these instabilities have been studied for frequencies less than the ion-beam gyrofrequency, with the exception of Goldstein and Wong (1987), and Brinca and Tsurutani (1988), who studied also the region of high frequencies (, where is the ion-beam gyrofrequency), in connection with pickup cometary ions. It has been recently demonstrated that in the cold plasma theory, left- and right-hand modes can be destabilized in a rather large range of frequency and wavenumber values. It has also been shown that, in some cases, the unstable spectrum has a band structure. We study here thermal effects on the cold modes and show that, as the temperature increases, the band structure becomes a double-humped unstable spectrum. For even larger temperatures, the double-humped structure is washed out, remaining a single-humped spectrum, but with an instability range which is similar to the cold plasma case. We then apply these results to the solar wind.
Lenguagedc.language.isoen
Sourcedc.sourcePlanetary and Space Science
Keywordsdc.subjectAstronomy and Astrophysics
Keywordsdc.subjectSpace and Planetary Science
Títulodc.titleElectromagnetic ion-beam-plasma instabilities
Document typedc.typeArtículo de revista
dcterms.accessRightsdcterms.accessRightsAcceso a solo metadatos
Catalogueruchile.catalogadorjmm
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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