Registro completo de metadatos
Campo DC | Valor | Lengua/Idioma |
---|---|---|
dc.provenance | Facultad de Ciencias Exactas y Naturales de la UBA | - |
dc.contributor | Greco, A. | - |
dc.contributor | Matthaeus, W.H. | - |
dc.contributor | Servidio, S. | - |
dc.contributor | Chuychai, P. | - |
dc.contributor | <div class="autor_fcen" id="2615">Dmitruk, P.</div> | - |
dc.creator | Greco, A. | - |
dc.creator | Matthaeus, W.H. | - |
dc.creator | Servidio, S. | - |
dc.creator | Chuychai, P. | - |
dc.creator | <div class="autor_fcen" id="2615">Dmitruk, P.</div> | - |
dc.date.accessioned | 2018-05-04T21:59:54Z | - |
dc.date.accessioned | 2018-05-28T15:49:33Z | - |
dc.date.available | 2018-05-04T21:59:54Z | - |
dc.date.available | 2018-05-28T15:49:33Z | - |
dc.date.issued | 2009 | - |
dc.identifier.uri | http://10.0.0.11:8080/jspui/handle/bnmm/68663 | - |
dc.description | The 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.description | Fil:Dmitruk, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. | - |
dc.format | application/pdf | - |
dc.language | eng | - |
dc.rights | info:eu-repo/semantics/openAccess | - |
dc.rights | http://creativecommons.org/licenses/by/2.5/ar | - |
dc.source | Astrophys. J. Lett. 2009;691(2):L111-L114 | - |
dc.source.uri | http://digital.bl.fcen.uba.ar/Download/paper/paper_20418205_v691_n2_pL111_Greco.pdf | - |
dc.subject | Interplanetary medium | - |
dc.subject | MHD | - |
dc.subject | Plasmas | - |
dc.subject | Solar wind | - |
dc.subject | Sun: magnetic fields | - |
dc.subject | Turbulence | - |
dc.title | Statistical analysis of discontinuities in solar wind ace data and comparison with intermittent mhd turbulence | - |
dc.type | info:eu-repo/semantics/article | - |
dc.type | info:ar-repo/semantics/artículo | - |
dc.type | info:eu-repo/semantics/publishedVersion | - |
Aparece en las colecciones: | FCEN - Facultad de Ciencias Exactas y Naturales. UBA |
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