Emergence of intermittent structures and reconnection in MHD turbulence

In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events...

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Detalles Bibliográficos
Autor principal: Dmitruk, Pablo Ariel
Publicado: 2010
Materias:
(magnetohydrodynamics:) MHD
(Sun:) solar wind
methods: numerical
turbulence
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v6_nS274_p116_Greco
http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS274_p116_Greco
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_17439213_v6_nS274_p116_Greco
record_format dspace
spelling paper:paper_17439213_v6_nS274_p116_Greco2023-06-08T16:28:03Z Emergence of intermittent structures and reconnection in MHD turbulence Dmitruk, Pablo Ariel (magnetohydrodynamics:) MHD (Sun:) solar wind methods: numerical turbulence In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union. Fil:Dmitruk, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2010 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v6_nS274_p116_Greco http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS274_p116_Greco
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic (magnetohydrodynamics:) MHD
(Sun:) solar wind
methods: numerical
turbulence
spellingShingle (magnetohydrodynamics:) MHD
(Sun:) solar wind
methods: numerical
turbulence
Dmitruk, Pablo Ariel
Emergence of intermittent structures and reconnection in MHD turbulence
topic_facet (magnetohydrodynamics:) MHD
(Sun:) solar wind
methods: numerical
turbulence
description In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union.
author Dmitruk, Pablo Ariel
author_facet Dmitruk, Pablo Ariel
author_sort Dmitruk, Pablo Ariel
title Emergence of intermittent structures and reconnection in MHD turbulence
title_short Emergence of intermittent structures and reconnection in MHD turbulence
title_full Emergence of intermittent structures and reconnection in MHD turbulence
title_fullStr Emergence of intermittent structures and reconnection in MHD turbulence
title_full_unstemmed Emergence of intermittent structures and reconnection in MHD turbulence
title_sort emergence of intermittent structures and reconnection in mhd turbulence
publishDate 2010
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v6_nS274_p116_Greco
http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS274_p116_Greco
work_keys_str_mv AT dmitrukpabloariel emergenceofintermittentstructuresandreconnectioninmhdturbulence
_version_ 1768546227958317056

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