Statistical analysis of discontinuities in solar wind ace data and comparison with intermittent mhd turbulence

dc.creatorGreco, A.
dc.creatorMatthaeus, W.H.
dc.creatorServidio, S.
dc.creatorChuychai, P.
dc.creatorDmitruk, Pablo Ariel
dc.date.accessioned2018-09-24T17:48:40Z
dc.date.accessioned2018-11-06T13:43:20Z
dc.date.available2018-09-24T17:48:40Z
dc.date.available2018-11-06T13:43:20Z
dc.date.created2018-09-24T17:48:40Z
dc.date.issued2009-12
dc.identifierGreco, A.; Matthaeus, W.H.; Servidio, S.; Chuychai, P.; Dmitruk, Pablo Ariel; Statistical analysis of discontinuities in solar wind ace data and comparison with intermittent mhd turbulence; IOP Publishing; Astrophysical Journal; 691; 2; 12-2009; 1141-1144
dc.identifier0004-637X
dc.identifierhttp://hdl.handle.net/11336/60764
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1878574
dc.description.abstractThe 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.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0004-637X/691/2/L111
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
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.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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