Intermittent MHD structures and classical discontinuities

dc.creatorGreco, Andres Francisco
dc.creatorChuychai, P.
dc.creatorMatthaeus, W.H.
dc.creatorServidio, S.
dc.creatorDmitruk, Pablo Ariel
dc.date.accessioned2018-10-11T16:04:43Z
dc.date.accessioned2018-11-06T14:09:30Z
dc.date.available2018-10-11T16:04:43Z
dc.date.available2018-11-06T14:09:30Z
dc.date.created2018-10-11T16:04:43Z
dc.date.issued2008-12
dc.identifierGreco, Andres Francisco; Chuychai, P.; Matthaeus, W.H.; Servidio, S.; Dmitruk, Pablo Ariel; Intermittent MHD structures and classical discontinuities; American Geophysical Union; Geophysical Research Letters; 35; 19; 12-2008; 191111-191114
dc.identifier0094-8276
dc.identifierhttp://hdl.handle.net/11336/62198
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1883401
dc.description.abstractWe examine statistics of rapid spatial variations of the magnetic field in simulations of magnetohydrodynamic (MHD) turbulence, by analyzing intermittency properties. and by using classical methods for identifying discontinuities. The methods identify similar structures, and give very similar event distribution functions. When the results are scaled to the correlation length, the average waiting times agree with typically reported waiting times between solar wind discontinuities. Thus discontinuities may be related to flux tube boundaries and intermittent structures that appear spontaneously in MHD turbulence. Copyright 2008 by the American Geophysical Union.
dc.languageeng
dc.publisherAmerican Geophysical Union
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1029/2008GL035454
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectmagnetohydrodynamic
dc.subjectturbulence
dc.titleIntermittent MHD structures and classical discontinuities
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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