Characterization of intermittent structures in the solar wind

The solar wind (SW) is a suitable natural scenario to study the intermittent nature of magnetohydrodynamic (MHD) turbulence for systems with low dissipation rate. In particular, nonlinear wave-wave interactions can be characterized by the degree of phase correlation and by departures from Gaussianit...

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Autores principales: Nakwacki, M.S., Ruiz, M.E., Dasso, S.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2013
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v8_nS300_p485_Nakwacki
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spelling paperaa:paper_17439213_v8_nS300_p485_Nakwacki2023-06-12T16:51:17Z Characterization of intermittent structures in the solar wind Proc. Int. Astron. Union 2013;8(S300):485-486 Nakwacki, M.S. Ruiz, M.E. Dasso, S. Intermittency Magnetohydrodynamic turbulence Solar Wind The solar wind (SW) is a suitable natural scenario to study the intermittent nature of magnetohydrodynamic (MHD) turbulence for systems with low dissipation rate. In particular, nonlinear wave-wave interactions can be characterized by the degree of phase correlation and by departures from Gaussianity of the magnetic field. In this work, we study in situ observations of magnetic field intensity from the spacecraft ACE, which is located near one astronomical unit from the Sun, in the SW near Earth. We compute the phase coherence index analyzing two sets of observations, each one consisting of approximately three months during 2008 and 2012, respectively. From these sets of data we characterize intermittent features of the magnetic field intensity corresponding to a solar maximum and a solar minimum. © 2013 International Astronomical Union. Fil:Nakwacki, M.S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Ruiz, M.E. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2013 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion application/pdf eng info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v8_nS300_p485_Nakwacki
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
language Inglés
orig_language_str_mv eng
topic Intermittency
Magnetohydrodynamic turbulence
Solar Wind
spellingShingle Intermittency
Magnetohydrodynamic turbulence
Solar Wind
Nakwacki, M.S.
Ruiz, M.E.
Dasso, S.
Characterization of intermittent structures in the solar wind
topic_facet Intermittency
Magnetohydrodynamic turbulence
Solar Wind
description The solar wind (SW) is a suitable natural scenario to study the intermittent nature of magnetohydrodynamic (MHD) turbulence for systems with low dissipation rate. In particular, nonlinear wave-wave interactions can be characterized by the degree of phase correlation and by departures from Gaussianity of the magnetic field. In this work, we study in situ observations of magnetic field intensity from the spacecraft ACE, which is located near one astronomical unit from the Sun, in the SW near Earth. We compute the phase coherence index analyzing two sets of observations, each one consisting of approximately three months during 2008 and 2012, respectively. From these sets of data we characterize intermittent features of the magnetic field intensity corresponding to a solar maximum and a solar minimum. © 2013 International Astronomical Union.
format Artículo
Artículo
publishedVersion
author Nakwacki, M.S.
Ruiz, M.E.
Dasso, S.
author_facet Nakwacki, M.S.
Ruiz, M.E.
Dasso, S.
author_sort Nakwacki, M.S.
title Characterization of intermittent structures in the solar wind
title_short Characterization of intermittent structures in the solar wind
title_full Characterization of intermittent structures in the solar wind
title_fullStr Characterization of intermittent structures in the solar wind
title_full_unstemmed Characterization of intermittent structures in the solar wind
title_sort characterization of intermittent structures in the solar wind
publishDate 2013
url http://hdl.handle.net/20.500.12110/paper_17439213_v8_nS300_p485_Nakwacki
work_keys_str_mv AT nakwackims characterizationofintermittentstructuresinthesolarwind
AT ruizme characterizationofintermittentstructuresinthesolarwind
AT dassos characterizationofintermittentstructuresinthesolarwind
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