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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Autores principales: Greco, A., Servidio, S., Matthaeus, W.H., Dmitruk, P.
Formato: SER
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS274_p116_Greco
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spelling todo:paper_17439213_v6_nS274_p116_Greco2023-10-03T16:31:36Z Emergence of intermittent structures and reconnection in MHD turbulence Greco, A. Servidio, S. Matthaeus, W.H. Dmitruk, P. (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. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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
Greco, A.
Servidio, S.
Matthaeus, W.H.
Dmitruk, P.
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.
format SER
author Greco, A.
Servidio, S.
Matthaeus, W.H.
Dmitruk, P.
author_facet Greco, A.
Servidio, S.
Matthaeus, W.H.
Dmitruk, P.
author_sort Greco, A.
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
url http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS274_p116_Greco
work_keys_str_mv AT grecoa emergenceofintermittentstructuresandreconnectioninmhdturbulence
AT servidios emergenceofintermittentstructuresandreconnectioninmhdturbulence
AT matthaeuswh emergenceofintermittentstructuresandreconnectioninmhdturbulence
AT dmitrukp emergenceofintermittentstructuresandreconnectioninmhdturbulence
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