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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/277477
Ver los metadatos del registro completo
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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 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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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 |
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eng |
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eng |
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openAccess |
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Wiley |
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