Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data
- Autores
- Osman, K.T.; Wan, M.; Matthaeus, W.H.; Weygand, J.M.; Dasso, S.
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The first direct determination of the inertial range energy cascade rate, using an anisotropic form of Yaglom's law for magnetohydrodynamic turbulence, is obtained in the solar wind with multispacecraft measurements. The two-point mixed third-order structure functions of Elsässer fluctuations are integrated over a sphere in magnetic field-aligned coordinates, and the result is consistent with a linear scaling. Therefore, volume integrated heating and cascade rates are obtained that, unlike previous studies, make only limited assumptions about the underlying spectral geometry of solar wind turbulence. These results confirm the turbulent nature of magnetic and velocity field fluctuations in the low frequency limit, and could supply the energy necessary to account for the nonadiabatic heating of the solar wind. © 2011 American Physical Society.
Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. - Fuente
- Phys Rev Lett 2011;107(16)
- Materia
-
Direct determination
Energy cascade
Linear scaling
Low frequency limits
Magnetohydrodynamic turbulence
Non-adiabatic
Solar-wind turbulence
Structure functions
Third-order
Two-point
Velocity field
Anisotropy
Heating
Magnetic fields
Magnetohydrodynamics
Solar wind
Spheres
Turbulence
Velocity
Solar energy - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/2.5/ar
- Repositorio
- Institución
- Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
- OAI Identificador
- paperaa:paper_00319007_v107_n16_p_Osman
Ver los metadatos del registro completo
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Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft dataOsman, K.T.Wan, M.Matthaeus, W.H.Weygand, J.M.Dasso, S.Direct determinationEnergy cascadeLinear scalingLow frequency limitsMagnetohydrodynamic turbulenceNon-adiabaticSolar-wind turbulenceStructure functionsThird-orderTwo-pointVelocity fieldAnisotropyHeatingMagnetic fieldsMagnetohydrodynamicsSolar windSpheresTurbulenceVelocitySolar energyThe first direct determination of the inertial range energy cascade rate, using an anisotropic form of Yaglom's law for magnetohydrodynamic turbulence, is obtained in the solar wind with multispacecraft measurements. The two-point mixed third-order structure functions of Elsässer fluctuations are integrated over a sphere in magnetic field-aligned coordinates, and the result is consistent with a linear scaling. Therefore, volume integrated heating and cascade rates are obtained that, unlike previous studies, make only limited assumptions about the underlying spectral geometry of solar wind turbulence. These results confirm the turbulent nature of magnetic and velocity field fluctuations in the low frequency limit, and could supply the energy necessary to account for the nonadiabatic heating of the solar wind. © 2011 American Physical Society.Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.2011info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://hdl.handle.net/20.500.12110/paper_00319007_v107_n16_p_OsmanPhys Rev Lett 2011;107(16)reponame:Biblioteca Digital (UBA-FCEN)instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesinstacron:UBA-FCENenginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/2.5/ar2025-09-29T13:42:55Zpaperaa:paper_00319007_v107_n16_p_OsmanInstitucionalhttps://digital.bl.fcen.uba.ar/Universidad públicaNo correspondehttps://digital.bl.fcen.uba.ar/cgi-bin/oaiserver.cgiana@bl.fcen.uba.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:18962025-09-29 13:42:56.444Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesfalse |
dc.title.none.fl_str_mv |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
title |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
spellingShingle |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data Osman, K.T. Direct determination Energy cascade Linear scaling Low frequency limits Magnetohydrodynamic turbulence Non-adiabatic Solar-wind turbulence Structure functions Third-order Two-point Velocity field Anisotropy Heating Magnetic fields Magnetohydrodynamics Solar wind Spheres Turbulence Velocity Solar energy |
title_short |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
title_full |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
title_fullStr |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
title_full_unstemmed |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
title_sort |
Anisotropic third-moment estimates of the energy cascade in solar wind turbulence using multispacecraft data |
dc.creator.none.fl_str_mv |
Osman, K.T. Wan, M. Matthaeus, W.H. Weygand, J.M. Dasso, S. |
author |
Osman, K.T. |
author_facet |
Osman, K.T. Wan, M. Matthaeus, W.H. Weygand, J.M. Dasso, S. |
author_role |
author |
author2 |
Wan, M. Matthaeus, W.H. Weygand, J.M. Dasso, S. |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Direct determination Energy cascade Linear scaling Low frequency limits Magnetohydrodynamic turbulence Non-adiabatic Solar-wind turbulence Structure functions Third-order Two-point Velocity field Anisotropy Heating Magnetic fields Magnetohydrodynamics Solar wind Spheres Turbulence Velocity Solar energy |
topic |
Direct determination Energy cascade Linear scaling Low frequency limits Magnetohydrodynamic turbulence Non-adiabatic Solar-wind turbulence Structure functions Third-order Two-point Velocity field Anisotropy Heating Magnetic fields Magnetohydrodynamics Solar wind Spheres Turbulence Velocity Solar energy |
dc.description.none.fl_txt_mv |
The first direct determination of the inertial range energy cascade rate, using an anisotropic form of Yaglom's law for magnetohydrodynamic turbulence, is obtained in the solar wind with multispacecraft measurements. The two-point mixed third-order structure functions of Elsässer fluctuations are integrated over a sphere in magnetic field-aligned coordinates, and the result is consistent with a linear scaling. Therefore, volume integrated heating and cascade rates are obtained that, unlike previous studies, make only limited assumptions about the underlying spectral geometry of solar wind turbulence. These results confirm the turbulent nature of magnetic and velocity field fluctuations in the low frequency limit, and could supply the energy necessary to account for the nonadiabatic heating of the solar wind. © 2011 American Physical Society. Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. |
description |
The first direct determination of the inertial range energy cascade rate, using an anisotropic form of Yaglom's law for magnetohydrodynamic turbulence, is obtained in the solar wind with multispacecraft measurements. The two-point mixed third-order structure functions of Elsässer fluctuations are integrated over a sphere in magnetic field-aligned coordinates, and the result is consistent with a linear scaling. Therefore, volume integrated heating and cascade rates are obtained that, unlike previous studies, make only limited assumptions about the underlying spectral geometry of solar wind turbulence. These results confirm the turbulent nature of magnetic and velocity field fluctuations in the low frequency limit, and could supply the energy necessary to account for the nonadiabatic heating of the solar wind. © 2011 American Physical Society. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/20.500.12110/paper_00319007_v107_n16_p_Osman |
url |
http://hdl.handle.net/20.500.12110/paper_00319007_v107_n16_p_Osman |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by/2.5/ar |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
Phys Rev Lett 2011;107(16) reponame:Biblioteca Digital (UBA-FCEN) instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales instacron:UBA-FCEN |
reponame_str |
Biblioteca Digital (UBA-FCEN) |
collection |
Biblioteca Digital (UBA-FCEN) |
instname_str |
Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales |
instacron_str |
UBA-FCEN |
institution |
UBA-FCEN |
repository.name.fl_str_mv |
Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales |
repository.mail.fl_str_mv |
ana@bl.fcen.uba.ar |
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1844618735490433024 |
score |
13.070432 |