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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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00319007_v93_n15_p155005_Milano |
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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 |
_version_ |
1807320051930365952 |