Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity

Autores
Andrés, Nahuel; Romanelli, Norberto Julio; Hadid, Lina Z.; Sahraoui, Fouad; DiBraccio, Gina; Halekas, Jasper
Año de publicación
2020
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The first estimation of the incompressible energy cascade rate at magnetohydrodynamic (MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of magnetic field and plasma observations provided by Mars Atmosphere and Volatile EvolutioN (MAVEN) over 600 orbits. In particular, the energy cascade rate is computed for events with and without proton cyclotron wave (PCW) activity, for time intervals when MAVEN was in the solar wind with no magnetic connection to the bow shock. It is shown that the nonlinear cascade of energy at the MHD scales is slightly amplified when PCWs are present in the plasma, around the Martian perihelion. In addition, the analysis of the normalized cross helicity and residual energy for the turbulent fluctuations shows the presence of Alfvénic and non-Alfvénic fluctuations in a magnetic dominant regime for the majority of the cases.
Fil: Andrés, Nahuel. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Romanelli, Norberto Julio. National Aeronautics and Space Administration; Estados Unidos. University of Maryland; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Hadid, Lina Z.. École Polytechnique; Francia. Sorbonne University; Francia. Agencia Espacial Europea. European Space Research And Technology Centre.; Países Bajos
Fil: Sahraoui, Fouad. École Polytechnique; Francia. Sorbonne University; Francia
Fil: DiBraccio, Gina. National Aeronautics and Space Administration; Estados Unidos
Fil: Halekas, Jasper. University of Iowa; Estados Unidos
Materia
Turbulencia
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/181813
Acceder
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves ActivityAndrés, NahuelRomanelli, Norberto JulioHadid, Lina Z.Sahraoui, FouadDiBraccio, GinaHalekas, JasperTurbulenciahttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The first estimation of the incompressible energy cascade rate at magnetohydrodynamic (MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of magnetic field and plasma observations provided by Mars Atmosphere and Volatile EvolutioN (MAVEN) over 600 orbits. In particular, the energy cascade rate is computed for events with and without proton cyclotron wave (PCW) activity, for time intervals when MAVEN was in the solar wind with no magnetic connection to the bow shock. It is shown that the nonlinear cascade of energy at the MHD scales is slightly amplified when PCWs are present in the plasma, around the Martian perihelion. In addition, the analysis of the normalized cross helicity and residual energy for the turbulent fluctuations shows the presence of Alfvénic and non-Alfvénic fluctuations in a magnetic dominant regime for the majority of the cases.Fil: Andrés, Nahuel. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Romanelli, Norberto Julio. National Aeronautics and Space Administration; Estados Unidos. University of Maryland; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Hadid, Lina Z.. École Polytechnique; Francia. Sorbonne University; Francia. Agencia Espacial Europea. European Space Research And Technology Centre.; Países BajosFil: Sahraoui, Fouad. École Polytechnique; Francia. Sorbonne University; FranciaFil: DiBraccio, Gina. National Aeronautics and Space Administration; Estados UnidosFil: Halekas, Jasper. University of Iowa; Estados UnidosIOP Publishing2020-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/181813Andrés, Nahuel; Romanelli, Norberto Julio; Hadid, Lina Z.; Sahraoui, Fouad; DiBraccio, Gina; et al.; Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity; IOP Publishing; Astrophysical Journal; 902; 2; 10-2020; 1-151538-43570004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/abb5a7info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/abb5a7info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2007.09476info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:49:36Zoai:ri.conicet.gov.ar:11336/181813instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:49:37.206CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
title Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
spellingShingle Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
Andrés, Nahuel
Turbulencia
title_short Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
title_full Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
title_fullStr Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
title_full_unstemmed Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
title_sort Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity
dc.creator.none.fl_str_mv Andrés, Nahuel
Romanelli, Norberto Julio
Hadid, Lina Z.
Sahraoui, Fouad
DiBraccio, Gina
Halekas, Jasper
author Andrés, Nahuel
author_facet Andrés, Nahuel
Romanelli, Norberto Julio
Hadid, Lina Z.
Sahraoui, Fouad
DiBraccio, Gina
Halekas, Jasper
author_role author
author2 Romanelli, Norberto Julio
Hadid, Lina Z.
Sahraoui, Fouad
DiBraccio, Gina
Halekas, Jasper
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Turbulencia
topic Turbulencia
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The first estimation of the incompressible energy cascade rate at magnetohydrodynamic (MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of magnetic field and plasma observations provided by Mars Atmosphere and Volatile EvolutioN (MAVEN) over 600 orbits. In particular, the energy cascade rate is computed for events with and without proton cyclotron wave (PCW) activity, for time intervals when MAVEN was in the solar wind with no magnetic connection to the bow shock. It is shown that the nonlinear cascade of energy at the MHD scales is slightly amplified when PCWs are present in the plasma, around the Martian perihelion. In addition, the analysis of the normalized cross helicity and residual energy for the turbulent fluctuations shows the presence of Alfvénic and non-Alfvénic fluctuations in a magnetic dominant regime for the majority of the cases.
Fil: Andrés, Nahuel. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Romanelli, Norberto Julio. National Aeronautics and Space Administration; Estados Unidos. University of Maryland; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Hadid, Lina Z.. École Polytechnique; Francia. Sorbonne University; Francia. Agencia Espacial Europea. European Space Research And Technology Centre.; Países Bajos
Fil: Sahraoui, Fouad. École Polytechnique; Francia. Sorbonne University; Francia
Fil: DiBraccio, Gina. National Aeronautics and Space Administration; Estados Unidos
Fil: Halekas, Jasper. University of Iowa; Estados Unidos
description The first estimation of the incompressible energy cascade rate at magnetohydrodynamic (MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of magnetic field and plasma observations provided by Mars Atmosphere and Volatile EvolutioN (MAVEN) over 600 orbits. In particular, the energy cascade rate is computed for events with and without proton cyclotron wave (PCW) activity, for time intervals when MAVEN was in the solar wind with no magnetic connection to the bow shock. It is shown that the nonlinear cascade of energy at the MHD scales is slightly amplified when PCWs are present in the plasma, around the Martian perihelion. In addition, the analysis of the normalized cross helicity and residual energy for the turbulent fluctuations shows the presence of Alfvénic and non-Alfvénic fluctuations in a magnetic dominant regime for the majority of the cases.
publishDate 2020
dc.date.none.fl_str_mv 2020-10
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/11336/181813
Andrés, Nahuel; Romanelli, Norberto Julio; Hadid, Lina Z.; Sahraoui, Fouad; DiBraccio, Gina; et al.; Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity; IOP Publishing; Astrophysical Journal; 902; 2; 10-2020; 1-15
1538-4357
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/181813
identifier_str_mv Andrés, Nahuel; Romanelli, Norberto Julio; Hadid, Lina Z.; Sahraoui, Fouad; DiBraccio, Gina; et al.; Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity; IOP Publishing; Astrophysical Journal; 902; 2; 10-2020; 1-15
1538-4357
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/abb5a7
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/abb5a7
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2007.09476
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1844613534803034112
score 13.070432

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