Spectral distribution of the cross helicity in the solar wind

Spectral distribution of the cross helicity in the solar wind was investigated. It was found that the space plasma turbulence is distributed anisotropically in space relative to magnetic field direction. The cross helicity was found to enter a magnetohydrodynamic description on equal footing with th...

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Autores principales: Milano, L.J., Dasso, S., Matthaeus, W.H., Smith, C.W.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00319007_v93_n15_p155005_Milano
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spelling todo:paper_00319007_v93_n15_p155005_Milano2023-10-03T14:43:13Z Spectral distribution of the cross helicity in the solar wind Milano, L.J. Dasso, S. Matthaeus, W.H. Smith, C.W. Anisotropy Heating Magnetic fields Magnetohydrodynamics Mathematical models Stability Thermal conductivity of solids Turbulence Vectors Cross helicity Solar wind Wave numbers Wave vectors Plasma theory Spectral distribution of the cross helicity in the solar wind was investigated. It was found that the space plasma turbulence is distributed anisotropically in space relative to magnetic field direction. The cross helicity was found to enter a magnetohydrodynamic description on equal footing with the energy. The rotational symmetry of the cross helicity was examined. It was found that the cross helicity is associated more or less equally with all angular components of the fluctuations. Fil:Milano, L.J. 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00319007_v93_n15_p155005_Milano
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Anisotropy
Heating
Magnetic fields
Magnetohydrodynamics
Mathematical models
Stability
Thermal conductivity of solids
Turbulence
Vectors
Cross helicity
Solar wind
Wave numbers
Wave vectors
Plasma theory
spellingShingle Anisotropy
Heating
Magnetic fields
Magnetohydrodynamics
Mathematical models
Stability
Thermal conductivity of solids
Turbulence
Vectors
Cross helicity
Solar wind
Wave numbers
Wave vectors
Plasma theory
Milano, L.J.
Dasso, S.
Matthaeus, W.H.
Smith, C.W.
Spectral distribution of the cross helicity in the solar wind
topic_facet Anisotropy
Heating
Magnetic fields
Magnetohydrodynamics
Mathematical models
Stability
Thermal conductivity of solids
Turbulence
Vectors
Cross helicity
Solar wind
Wave numbers
Wave vectors
Plasma theory
description Spectral distribution of the cross helicity in the solar wind was investigated. It was found that the space plasma turbulence is distributed anisotropically in space relative to magnetic field direction. The cross helicity was found to enter a magnetohydrodynamic description on equal footing with the energy. The rotational symmetry of the cross helicity was examined. It was found that the cross helicity is associated more or less equally with all angular components of the fluctuations.
format JOUR
author Milano, L.J.
Dasso, S.
Matthaeus, W.H.
Smith, C.W.
author_facet Milano, L.J.
Dasso, S.
Matthaeus, W.H.
Smith, C.W.
author_sort Milano, L.J.
title Spectral distribution of the cross helicity in the solar wind
title_short Spectral distribution of the cross helicity in the solar wind
title_full Spectral distribution of the cross helicity in the solar wind
title_fullStr Spectral distribution of the cross helicity in the solar wind
title_full_unstemmed Spectral distribution of the cross helicity in the solar wind
title_sort spectral distribution of the cross helicity in the solar wind
url http://hdl.handle.net/20.500.12110/paper_00319007_v93_n15_p155005_Milano
work_keys_str_mv AT milanolj spectraldistributionofthecrosshelicityinthesolarwind
AT dassos spectraldistributionofthecrosshelicityinthesolarwind
AT matthaeuswh spectraldistributionofthecrosshelicityinthesolarwind
AT smithcw spectraldistributionofthecrosshelicityinthesolarwind
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