Interplanetary magnetic Taylor microscale and implications for plasma dissipation

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The Taylor microscale, a measure of mean square spatial derivatives, is evaluated for interplanetary magnetic field fluctuations from single- and multiple-point data using Cluster and ACE spacecraft data. The Taylor scale is compared to the measured inner scale, which for hydrodynamics would corresp...

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Autores principales:	Matthaeus, W.H., Weygand, J.M., Chuychai, P., Dasso, S., Smith, C.W., Kivelson, M.G.
Formato:	Artículo publishedVersion
Publicado:	2008
Materias:	Interplanetary medium Magnetic fields Methods: data analysis Plasmas Solar wind Turbulence
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v678_n2PART2_pL141_Matthaeus https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v678_n2PART2_pL141_Matthaeus_oai
Aporte de:	Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

id	I28-R145-paper_0004637X_v678_n2PART2_pL141_Matthaeus_oai
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spelling	I28-R145-paper_0004637X_v678_n2PART2_pL141_Matthaeus_oai2024-08-16 Matthaeus, W.H. Weygand, J.M. Chuychai, P. Dasso, S. Smith, C.W. Kivelson, M.G. 2008 The Taylor microscale, a measure of mean square spatial derivatives, is evaluated for interplanetary magnetic field fluctuations from single- and multiple-point data using Cluster and ACE spacecraft data. The Taylor scale is compared to the measured inner scale, which for hydrodynamics would correspond to the Kolmogorov scale. The results are not consistent with dissipation of the hydrodynamic type, and indicate that solar wind dissipation involves kinetic plasma physics at both proton and electron scales. © 2008. The American Astronomical Society. All rights reserved. Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. application/pdf http://hdl.handle.net/20.500.12110/paper_0004637X_v678_n2PART2_pL141_Matthaeus info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar Astrophys. J. 2008;678(2 PART 2):L141-L144 Interplanetary medium Magnetic fields Methods: data analysis Plasmas Solar wind Turbulence Interplanetary magnetic Taylor microscale and implications for plasma dissipation info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v678_n2PART2_pL141_Matthaeus_oai
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-145
collection	Repositorio Digital de la Universidad de Buenos Aires (UBA)
topic	Interplanetary medium Magnetic fields Methods: data analysis Plasmas Solar wind Turbulence
spellingShingle	Interplanetary medium Magnetic fields Methods: data analysis Plasmas Solar wind Turbulence Matthaeus, W.H. Weygand, J.M. Chuychai, P. Dasso, S. Smith, C.W. Kivelson, M.G. Interplanetary magnetic Taylor microscale and implications for plasma dissipation
topic_facet	Interplanetary medium Magnetic fields Methods: data analysis Plasmas Solar wind Turbulence
description	The Taylor microscale, a measure of mean square spatial derivatives, is evaluated for interplanetary magnetic field fluctuations from single- and multiple-point data using Cluster and ACE spacecraft data. The Taylor scale is compared to the measured inner scale, which for hydrodynamics would correspond to the Kolmogorov scale. The results are not consistent with dissipation of the hydrodynamic type, and indicate that solar wind dissipation involves kinetic plasma physics at both proton and electron scales. © 2008. The American Astronomical Society. All rights reserved.
format	Artículo Artículo publishedVersion
author	Matthaeus, W.H. Weygand, J.M. Chuychai, P. Dasso, S. Smith, C.W. Kivelson, M.G.
author_facet	Matthaeus, W.H. Weygand, J.M. Chuychai, P. Dasso, S. Smith, C.W. Kivelson, M.G.
author_sort	Matthaeus, W.H.
title	Interplanetary magnetic Taylor microscale and implications for plasma dissipation
title_short	Interplanetary magnetic Taylor microscale and implications for plasma dissipation
title_full	Interplanetary magnetic Taylor microscale and implications for plasma dissipation
title_fullStr	Interplanetary magnetic Taylor microscale and implications for plasma dissipation
title_full_unstemmed	Interplanetary magnetic Taylor microscale and implications for plasma dissipation
title_sort	interplanetary magnetic taylor microscale and implications for plasma dissipation
publishDate	2008
url	http://hdl.handle.net/20.500.12110/paper_0004637X_v678_n2PART2_pL141_Matthaeus https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v678_n2PART2_pL141_Matthaeus_oai
work_keys_str_mv	AT matthaeuswh interplanetarymagnetictaylormicroscaleandimplicationsforplasmadissipation AT weygandjm interplanetarymagnetictaylormicroscaleandimplicationsforplasmadissipation AT chuychaip interplanetarymagnetictaylormicroscaleandimplicationsforplasmadissipation AT dassos interplanetarymagnetictaylormicroscaleandimplicationsforplasmadissipation AT smithcw interplanetarymagnetictaylormicroscaleandimplicationsforplasmadissipation AT kivelsonmg interplanetarymagnetictaylormicroscaleandimplicationsforplasmadissipation
_version_	1809356768506019840

Interplanetary magnetic Taylor microscale and implications for plasma dissipation

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