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Authordc.contributor.authorGomberoff, L. 
Authordc.contributor.authorAraneda, J. A. 
Admission datedc.date.accessioned2019-01-29T15:32:22Z
Available datedc.date.available2019-01-29T15:32:22Z
Publication datedc.date.issued2001
Cita de ítemdc.identifier.citationAstrophysics and Space Science, Volumen 277, Issue 1-2, 2018, Pages 103-106
Identifierdc.identifier.issn0004640X
Identifierdc.identifier.other10.1023/A:1012280010934
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/161636
Abstractdc.description.abstractIt is shown that damping effects can destabilize regions that are stable under non-dissipative fluid theory. Damping effects on the ion-acoustic modes are simulated by a collisional-like term in the longitudinal component of the fluid equations. It is shown that when there is only a beat wave instability, damping effects can destabilize modulational and decay-type instabilities. These results are in agreement with hybrid kinetic-fluid approaches and hybrid simulation codes.
Lenguagedc.language.isoen
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourceAstrophysics and Space Science
Keywordsdc.subjectAstronomy and Astrophysics
Keywordsdc.subjectSpace and Planetary Science
Títulodc.titleDamping effects on parametric decays of Alfvén waves
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorSCOPUS
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