Local Generation of Mirror Modes by Pickup Protons at Mars

Autores
Simon Wedlund, C.; Mazelle, C.; Meziane, K.; Bertucci, Cesar; Volwerk, M.; Preisser, L.; Schmid, D.; Halekas, J.; McFadden, J.; Mitchell, D.; Espley, J.; Henri, P.
Año de publicación
2025
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Mirror mode structures are born from a plasma instability driven by a large temperature anisotropy and appear downstream of planetary and interplanetary shocks, in their magnetosheath. As so-called “magnetic bottles” imprisoning dense and hot plasma, they are usually observed downstream of their region of formation, where the anisotropy is large and free energy is available, implying that they are advected with the plasma flow to the detection region. At Earth and other planets, the quasi-perpendicular shock provides the plasma with the necessary heating along the perpendicular direction to the local magnetic field. At Mars, which boasts an extended exosphere, an additional source of temperature anisotropy exists, through unstable ring-beam velocity distributions, that is, through ions locally ionized and subsequently picked up by the local electric fields. We report here for the first time an example of near locally-generated mirror mode structures due to pickup protons at Mars using the full plasma instrument suite on board the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. We present events with mirror modes in quasi-perpendicular and quasi-parallel shock conditions, discuss the locality of their generation and show that, in addition to the classic quasi-perpendicular source of anisotropy, another source exists, that is, unstable pickup protons. The existence at Mars of this extra ion anisotropy-generating mechanism is reminiscent of comets.
Fil: Simon Wedlund, C.. Austrian Academy Of Sciences;
Fil: Mazelle, C.. Centre National de la Recherche Scientifique; Francia
Fil: Meziane, K.. University Of New Brunswick.; Canadá
Fil: Bertucci, Cesar. 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: Volwerk, M.. Austrian Academy Of Sciences;
Fil: Preisser, L.. Université d Orléans; Francia
Fil: Schmid, D.. Austrian Academy Of Sciences;
Fil: Halekas, J.. University of Iowa; Estados Unidos
Fil: McFadden, J.. University of California at Berkeley; Estados Unidos
Fil: Mitchell, D.. University of California at Berkeley; Estados Unidos
Fil: Espley, J.. No especifíca;
Fil: Henri, P.. No especifíca;
Materia
MARS
WAVES
MIRROR MODES
MAGNETOSPHERE
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:11336/277477

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network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Local Generation of Mirror Modes by Pickup Protons at MarsSimon Wedlund, C.Mazelle, C.Meziane, K.Bertucci, CesarVolwerk, M.Preisser, L.Schmid, D.Halekas, J.McFadden, J.Mitchell, D.Espley, J.Henri, P.MARSWAVESMIRROR MODESMAGNETOSPHEREhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Mirror mode structures are born from a plasma instability driven by a large temperature anisotropy and appear downstream of planetary and interplanetary shocks, in their magnetosheath. As so-called “magnetic bottles” imprisoning dense and hot plasma, they are usually observed downstream of their region of formation, where the anisotropy is large and free energy is available, implying that they are advected with the plasma flow to the detection region. At Earth and other planets, the quasi-perpendicular shock provides the plasma with the necessary heating along the perpendicular direction to the local magnetic field. At Mars, which boasts an extended exosphere, an additional source of temperature anisotropy exists, through unstable ring-beam velocity distributions, that is, through ions locally ionized and subsequently picked up by the local electric fields. We report here for the first time an example of near locally-generated mirror mode structures due to pickup protons at Mars using the full plasma instrument suite on board the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. We present events with mirror modes in quasi-perpendicular and quasi-parallel shock conditions, discuss the locality of their generation and show that, in addition to the classic quasi-perpendicular source of anisotropy, another source exists, that is, unstable pickup protons. The existence at Mars of this extra ion anisotropy-generating mechanism is reminiscent of comets.Fil: Simon Wedlund, C.. Austrian Academy Of Sciences;Fil: Mazelle, C.. Centre National de la Recherche Scientifique; FranciaFil: Meziane, K.. University Of New Brunswick.; CanadáFil: Bertucci, Cesar. 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: Volwerk, M.. Austrian Academy Of Sciences;Fil: Preisser, L.. Université d Orléans; FranciaFil: Schmid, D.. Austrian Academy Of Sciences;Fil: Halekas, J.. University of Iowa; Estados UnidosFil: McFadden, J.. University of California at Berkeley; Estados UnidosFil: Mitchell, D.. University of California at Berkeley; Estados UnidosFil: Espley, J.. No especifíca;Fil: Henri, P.. No especifíca;Wiley2025-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/277477Simon Wedlund, C.; Mazelle, C.; Meziane, K.; Bertucci, Cesar; Volwerk, M.; et al.; Local Generation of Mirror Modes by Pickup Protons at Mars; Wiley; Journal of Geophysical Research: Space Physics; 130; 1; 1-2025; 1-202169-93802169-9402CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JA033275info:eu-repo/semantics/altIdentifier/doi/10.1029/2024JA033275info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-12-23T14:06:34Zoai:ri.conicet.gov.ar:11336/277477instacron: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:34982025-12-23 14:06:35.093CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Local Generation of Mirror Modes by Pickup Protons at Mars
title Local Generation of Mirror Modes by Pickup Protons at Mars
spellingShingle Local Generation of Mirror Modes by Pickup Protons at Mars
Simon Wedlund, C.
MARS
WAVES
MIRROR MODES
MAGNETOSPHERE
title_short Local Generation of Mirror Modes by Pickup Protons at Mars
title_full Local Generation of Mirror Modes by Pickup Protons at Mars
title_fullStr Local Generation of Mirror Modes by Pickup Protons at Mars
title_full_unstemmed Local Generation of Mirror Modes by Pickup Protons at Mars
title_sort Local Generation of Mirror Modes by Pickup Protons at Mars
dc.creator.none.fl_str_mv Simon Wedlund, C.
Mazelle, C.
Meziane, K.
Bertucci, Cesar
Volwerk, M.
Preisser, L.
Schmid, D.
Halekas, J.
McFadden, J.
Mitchell, D.
Espley, J.
Henri, P.
author Simon Wedlund, C.
author_facet Simon Wedlund, C.
Mazelle, C.
Meziane, K.
Bertucci, Cesar
Volwerk, M.
Preisser, L.
Schmid, D.
Halekas, J.
McFadden, J.
Mitchell, D.
Espley, J.
Henri, P.
author_role author
author2 Mazelle, C.
Meziane, K.
Bertucci, Cesar
Volwerk, M.
Preisser, L.
Schmid, D.
Halekas, J.
McFadden, J.
Mitchell, D.
Espley, J.
Henri, P.
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv MARS
WAVES
MIRROR MODES
MAGNETOSPHERE
topic MARS
WAVES
MIRROR MODES
MAGNETOSPHERE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Mirror mode structures are born from a plasma instability driven by a large temperature anisotropy and appear downstream of planetary and interplanetary shocks, in their magnetosheath. As so-called “magnetic bottles” imprisoning dense and hot plasma, they are usually observed downstream of their region of formation, where the anisotropy is large and free energy is available, implying that they are advected with the plasma flow to the detection region. At Earth and other planets, the quasi-perpendicular shock provides the plasma with the necessary heating along the perpendicular direction to the local magnetic field. At Mars, which boasts an extended exosphere, an additional source of temperature anisotropy exists, through unstable ring-beam velocity distributions, that is, through ions locally ionized and subsequently picked up by the local electric fields. We report here for the first time an example of near locally-generated mirror mode structures due to pickup protons at Mars using the full plasma instrument suite on board the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. We present events with mirror modes in quasi-perpendicular and quasi-parallel shock conditions, discuss the locality of their generation and show that, in addition to the classic quasi-perpendicular source of anisotropy, another source exists, that is, unstable pickup protons. The existence at Mars of this extra ion anisotropy-generating mechanism is reminiscent of comets.
Fil: Simon Wedlund, C.. Austrian Academy Of Sciences;
Fil: Mazelle, C.. Centre National de la Recherche Scientifique; Francia
Fil: Meziane, K.. University Of New Brunswick.; Canadá
Fil: Bertucci, Cesar. 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: Volwerk, M.. Austrian Academy Of Sciences;
Fil: Preisser, L.. Université d Orléans; Francia
Fil: Schmid, D.. Austrian Academy Of Sciences;
Fil: Halekas, J.. University of Iowa; Estados Unidos
Fil: McFadden, J.. University of California at Berkeley; Estados Unidos
Fil: Mitchell, D.. University of California at Berkeley; Estados Unidos
Fil: Espley, J.. No especifíca;
Fil: Henri, P.. No especifíca;
description Mirror mode structures are born from a plasma instability driven by a large temperature anisotropy and appear downstream of planetary and interplanetary shocks, in their magnetosheath. As so-called “magnetic bottles” imprisoning dense and hot plasma, they are usually observed downstream of their region of formation, where the anisotropy is large and free energy is available, implying that they are advected with the plasma flow to the detection region. At Earth and other planets, the quasi-perpendicular shock provides the plasma with the necessary heating along the perpendicular direction to the local magnetic field. At Mars, which boasts an extended exosphere, an additional source of temperature anisotropy exists, through unstable ring-beam velocity distributions, that is, through ions locally ionized and subsequently picked up by the local electric fields. We report here for the first time an example of near locally-generated mirror mode structures due to pickup protons at Mars using the full plasma instrument suite on board the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. We present events with mirror modes in quasi-perpendicular and quasi-parallel shock conditions, discuss the locality of their generation and show that, in addition to the classic quasi-perpendicular source of anisotropy, another source exists, that is, unstable pickup protons. The existence at Mars of this extra ion anisotropy-generating mechanism is reminiscent of comets.
publishDate 2025
dc.date.none.fl_str_mv 2025-01
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/11336/277477
Simon Wedlund, C.; Mazelle, C.; Meziane, K.; Bertucci, Cesar; Volwerk, M.; et al.; Local Generation of Mirror Modes by Pickup Protons at Mars; Wiley; Journal of Geophysical Research: Space Physics; 130; 1; 1-2025; 1-20
2169-9380
2169-9402
CONICET Digital
CONICET
url http://hdl.handle.net/11336/277477
identifier_str_mv Simon Wedlund, C.; Mazelle, C.; Meziane, K.; Bertucci, Cesar; Volwerk, M.; et al.; Local Generation of Mirror Modes by Pickup Protons at Mars; Wiley; Journal of Geophysical Research: Space Physics; 130; 1; 1-2025; 1-20
2169-9380
2169-9402
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://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JA033275
info:eu-repo/semantics/altIdentifier/doi/10.1029/2024JA033275
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
dc.publisher.none.fl_str_mv Wiley
publisher.none.fl_str_mv Wiley
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
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