dc.creatorGomberoff, L.
dc.creatorHoyos, J.
dc.creatorBrinca, A. L.
dc.date.accessioned2019-01-29T13:47:37Z
dc.date.available2019-01-29T13:47:37Z
dc.date.created2019-01-29T13:47:37Z
dc.date.issued2005
dc.identifierJournal of Geophysical Research: Space Physics, Volumen 110, Issue A6, 2005.
dc.identifier21699402
dc.identifier10.1029/2004JA010810
dc.identifierhttp://repositorio.uchile.cl/handle/2250/159772
dc.description.abstract[1] It is shown that ion-acoustic waves propagating along an external magnetic field and generated by parametric decays of circularly polarized finite amplitude waves have the properties of ion-acoustic waves observed in the solar wind.
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.titleIon acoustic instability triggered by finite amplitude polarized waves in the solar wind
dc.typeArtículos de revistas


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