dc.creatorGomberoff, L.
dc.date.accessioned2019-01-29T15:34:36Z
dc.date.available2019-01-29T15:34:36Z
dc.date.created2019-01-29T15:34:36Z
dc.date.issued2007
dc.identifierJournal of Geophysical Research: Space Physics, Volumen 112, Issue 10, 2018,
dc.identifier21699402
dc.identifier10.1029/2007JA012529
dc.identifierhttps://repositorio.uchile.cl/handle/2250/161674
dc.description.abstractThe effects of a finite-amplitude Alfvén wave in a plasma system with a proton and an alpha-particle beam, are studied. The system is described by a fourteenth-order polynomial providing, thereby, many decay channels for the finite-amplitude Alfvén wave. Apart from the parametric decays, the finite-amplitude wave affects very drastically the stability properties of the linear system. It is shown that the large-amplitude waves can either stabilize or destabilize further linear magnetosonic and ion-cyclotron instabilities like in the case of one ion beam. However, as opposed to the case of one ion beam, for large enough amplitude of the finite-amplitude wave, the effect on the linear system is always stabilizing. The finite-amplitude waves can also trigger nonlinear purely electrostatic ion-acoustic-like instabilities. However, in the present case, even forward propagating Alfvén waves can destabilize electrostatic waves supported by the beams, something that does not happen when there i
dc.languageen
dc.publisherBlackwell Publishing Ltd
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceJournal of Geophysical Research: Space Physics
dc.subjectGeophysics
dc.subjectOceanography
dc.subjectForestry
dc.subjectEcology
dc.subjectAquatic Science
dc.subjectWater Science and Technology
dc.subjectSoil Science
dc.subjectGeochemistry and Petrology
dc.subjectEarth-Surface Processes
dc.subjectAtmospheric Science
dc.subjectEarth and Planetary Sciences (miscellaneous)
dc.subjectSpace and Planetary Science
dc.subjectPaleontology
dc.titleParametric decays, stabilization effects, and electrostatic instabilities due to finite-amplitude Alfvén waves in a fast solar wind-like plasma
dc.typeArtículo de revista


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