Registro completo de metadatos
Campo DC Valor Lengua/Idioma
dc.provenanceFacultad de Ciencias Exactas y Naturales de la UBA-
dc.contributorGreco, A.-
dc.contributorMatthaeus, W.H.-
dc.contributorServidio, S.-
dc.contributorChuychai, P.-
dc.contributor<div class="autor_fcen" id="2615">Dmitruk, P.</div>-
dc.creatorGreco, A.-
dc.creatorMatthaeus, W.H.-
dc.creatorServidio, S.-
dc.creatorChuychai, P.-
dc.creator<div class="autor_fcen" id="2615">Dmitruk, P.</div>-
dc.date.accessioned2018-05-04T21:59:54Z-
dc.date.accessioned2018-05-28T15:49:33Z-
dc.date.available2018-05-04T21:59:54Z-
dc.date.available2018-05-28T15:49:33Z-
dc.date.issued2009-
dc.identifier.urihttp://10.0.0.11:8080/jspui/handle/bnmm/68663-
dc.descriptionThe comparison between Advanced Composition Explorer (ACE) solar wind data and simulations of magnetohydrodynamic (MHD) turbulence shows a good agreement in the waiting-time analysis of magnetic field increments. Similarity between classical discontinuity identification and intermittency analysis suggests a dynamical connection between solar wind discontinuities and intermittent MHD turbulence. Probability distribution functions of increments in ACE data and in simulations reveal a robust structure consisting of small random currents, current cores, and intermittent current sheets. This adds to evidence that solar wind magnetic structures may emerge fast and locally from MHD turbulence. © 2009. The American Astronomical Society. All rights reserved..-
dc.descriptionFil:Dmitruk, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.-
dc.formatapplication/pdf-
dc.languageeng-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttp://creativecommons.org/licenses/by/2.5/ar-
dc.sourceAstrophys. J. Lett. 2009;691(2):L111-L114-
dc.source.urihttp://digital.bl.fcen.uba.ar/Download/paper/paper_20418205_v691_n2_pL111_Greco.pdf-
dc.subjectInterplanetary medium-
dc.subjectMHD-
dc.subjectPlasmas-
dc.subjectSolar wind-
dc.subjectSun: magnetic fields-
dc.subjectTurbulence-
dc.titleStatistical analysis of discontinuities in solar wind ace data and comparison with intermittent mhd turbulence-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:ar-repo/semantics/artículo-
dc.typeinfo:eu-repo/semantics/publishedVersion-
Aparece en las colecciones: FCEN - Facultad de Ciencias Exactas y Naturales. UBA

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