Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation”
- Autores
- Sánchez Cano, Beatriz; Lester, Mark; Andrews, David J.; Opgenoorth, Hermann; Lillis, Robert; Leblanc, François; Fowler, Christopher M.; Fang, Xiaohua; Vaisberg, Oleg; Mayyasi, Majd; Holmberg, Mika; Guo, Jingnan; Hamrin, Maria; Mazelle, Christian; Peter, Kerstin; Pätzold, Martin; Stergiopoulou, Katerina; Goetz, Charlotte; Ermakov, Vladimir Nikolaevich; Shuvalov, Sergei; Wild, James A.; Blelly, Pierre Louis; Mendillo, Michael; Bertucci, Cesar; Cartacci, Marco; Orosei, Roberto; Chu, Feng; Kopf, Andrew J.; Girazian, Zachary; Roman, Michael T.
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The objective of this White Paper, submitted to ESA’s Voyage 2050 call, is to get a more holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the undisturbed solar wind outside of the induced magnetosphere. This can only be achieved with coordinated multi-point observations with high temporal resolution as they have the scientific potential to track the whole dynamics of the system (from small to large scales), and they constitute the next generation of the exploration of Mars analogous to what happened at Earth a few decades ago. This White Paper discusses the key science questions that are still open at Mars and how they could be addressed with coordinated multipoint missions. The main science questions are: (i) How does solar wind driving impact the dynamics of the magnetosphere and ionosphere? (ii) What is the structure and nature of the tail of Mars’ magnetosphere at all scales? (iii) How does the lower atmosphere couple to the upper atmosphere? (iv) Why should we have a permanent in-situ Space Weather monitor at Mars? Each science question is devoted to a specific plasma region, and includes several specific scientific objectives to study in the coming decades. In addition, two mission concepts are also proposed based on coordinated multi-point science from a constellation of orbiting and ground-based platforms, which focus on understanding and solving the current science gaps.
Fil: Sánchez Cano, Beatriz. University of Leicester; Reino Unido
Fil: Lester, Mark. University of Leicester; Reino Unido
Fil: Andrews, David J.. No especifíca;
Fil: Opgenoorth, Hermann. Universidad de Umea; Suecia. University of Leicester; Reino Unido
Fil: Lillis, Robert. No especifíca;
Fil: Leblanc, François. Université Pierre et Marie Curie; Francia
Fil: Fowler, Christopher M.. No especifíca;
Fil: Fang, Xiaohua. State University of Colorado at Boulder; Estados Unidos
Fil: Vaisberg, Oleg. Space Research Institute Of The Russian Academy Of Sciences; Rusia
Fil: Mayyasi, Majd. Boston University; Estados Unidos
Fil: Holmberg, Mika. No especifíca;
Fil: Guo, Jingnan. Chinese Academy of Sciences; República de China
Fil: Hamrin, Maria. Universidad de Umea; Suecia
Fil: Mazelle, Christian. No especifíca;
Fil: Peter, Kerstin. Universitat zu Köln; Alemania
Fil: Pätzold, Martin. Universitat zu Köln; Alemania
Fil: Stergiopoulou, Katerina. No especifíca;
Fil: Goetz, Charlotte. No especifíca;
Fil: Ermakov, Vladimir Nikolaevich. No especifíca;
Fil: Shuvalov, Sergei. Space Research Institute Of The Russian Academy Of Sciences; Rusia
Fil: Wild, James A.. Lancaster University; Reino Unido
Fil: Blelly, Pierre Louis. No especifíca;
Fil: Mendillo, Michael. Boston University; Estados Unidos
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: Cartacci, Marco. Istituto Nazionale di Astrofisica; Italia
Fil: Orosei, Roberto. Istituto Di Radioastronomia; Italia
Fil: Chu, Feng. University of Iowa; Estados Unidos
Fil: Kopf, Andrew J.. No especifíca;
Fil: Girazian, Zachary. University of Iowa; Estados Unidos
Fil: Roman, Michael T.. University of Leicester; Reino Unido - Materia
-
COORDINATED MULTIPOINT MISSIONS
ESA-VOYAGE2050
FUTURE MISSIONS
MARS
PLASMA
SCIENCE GAPS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/212538
Ver los metadatos del registro completo
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Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation”Sánchez Cano, BeatrizLester, MarkAndrews, David J.Opgenoorth, HermannLillis, RobertLeblanc, FrançoisFowler, Christopher M.Fang, XiaohuaVaisberg, OlegMayyasi, MajdHolmberg, MikaGuo, JingnanHamrin, MariaMazelle, ChristianPeter, KerstinPätzold, MartinStergiopoulou, KaterinaGoetz, CharlotteErmakov, Vladimir NikolaevichShuvalov, SergeiWild, James A.Blelly, Pierre LouisMendillo, MichaelBertucci, CesarCartacci, MarcoOrosei, RobertoChu, FengKopf, Andrew J.Girazian, ZacharyRoman, Michael T.COORDINATED MULTIPOINT MISSIONSESA-VOYAGE2050FUTURE MISSIONSMARSPLASMASCIENCE GAPShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The objective of this White Paper, submitted to ESA’s Voyage 2050 call, is to get a more holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the undisturbed solar wind outside of the induced magnetosphere. This can only be achieved with coordinated multi-point observations with high temporal resolution as they have the scientific potential to track the whole dynamics of the system (from small to large scales), and they constitute the next generation of the exploration of Mars analogous to what happened at Earth a few decades ago. This White Paper discusses the key science questions that are still open at Mars and how they could be addressed with coordinated multipoint missions. The main science questions are: (i) How does solar wind driving impact the dynamics of the magnetosphere and ionosphere? (ii) What is the structure and nature of the tail of Mars’ magnetosphere at all scales? (iii) How does the lower atmosphere couple to the upper atmosphere? (iv) Why should we have a permanent in-situ Space Weather monitor at Mars? Each science question is devoted to a specific plasma region, and includes several specific scientific objectives to study in the coming decades. In addition, two mission concepts are also proposed based on coordinated multi-point science from a constellation of orbiting and ground-based platforms, which focus on understanding and solving the current science gaps.Fil: Sánchez Cano, Beatriz. University of Leicester; Reino UnidoFil: Lester, Mark. University of Leicester; Reino UnidoFil: Andrews, David J.. No especifíca;Fil: Opgenoorth, Hermann. Universidad de Umea; Suecia. University of Leicester; Reino UnidoFil: Lillis, Robert. No especifíca;Fil: Leblanc, François. Université Pierre et Marie Curie; FranciaFil: Fowler, Christopher M.. No especifíca;Fil: Fang, Xiaohua. State University of Colorado at Boulder; Estados UnidosFil: Vaisberg, Oleg. Space Research Institute Of The Russian Academy Of Sciences; RusiaFil: Mayyasi, Majd. Boston University; Estados UnidosFil: Holmberg, Mika. No especifíca;Fil: Guo, Jingnan. Chinese Academy of Sciences; República de ChinaFil: Hamrin, Maria. Universidad de Umea; SueciaFil: Mazelle, Christian. No especifíca;Fil: Peter, Kerstin. Universitat zu Köln; AlemaniaFil: Pätzold, Martin. Universitat zu Köln; AlemaniaFil: Stergiopoulou, Katerina. No especifíca;Fil: Goetz, Charlotte. No especifíca;Fil: Ermakov, Vladimir Nikolaevich. No especifíca;Fil: Shuvalov, Sergei. Space Research Institute Of The Russian Academy Of Sciences; RusiaFil: Wild, James A.. Lancaster University; Reino UnidoFil: Blelly, Pierre Louis. No especifíca;Fil: Mendillo, Michael. Boston University; Estados UnidosFil: 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: Cartacci, Marco. Istituto Nazionale di Astrofisica; ItaliaFil: Orosei, Roberto. Istituto Di Radioastronomia; ItaliaFil: Chu, Feng. University of Iowa; Estados UnidosFil: Kopf, Andrew J.. No especifíca;Fil: Girazian, Zachary. University of Iowa; Estados UnidosFil: Roman, Michael T.. University of Leicester; Reino UnidoSpringer2021-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/212538Sánchez Cano, Beatriz; Lester, Mark; Andrews, David J.; Opgenoorth, Hermann; Lillis, Robert; et al.; Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation”; Springer; Experimental Astronomy; 54; 2-3; 11-2021; 641-6760922-6435CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-021-09790-0info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-17T11:01:38Zoai:ri.conicet.gov.ar:11336/212538instacron: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:34982025-09-17 11:01:38.658CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
title |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
spellingShingle |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” Sánchez Cano, Beatriz COORDINATED MULTIPOINT MISSIONS ESA-VOYAGE2050 FUTURE MISSIONS MARS PLASMA SCIENCE GAPS |
title_short |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
title_full |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
title_fullStr |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
title_full_unstemmed |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
title_sort |
Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation” |
dc.creator.none.fl_str_mv |
Sánchez Cano, Beatriz Lester, Mark Andrews, David J. Opgenoorth, Hermann Lillis, Robert Leblanc, François Fowler, Christopher M. Fang, Xiaohua Vaisberg, Oleg Mayyasi, Majd Holmberg, Mika Guo, Jingnan Hamrin, Maria Mazelle, Christian Peter, Kerstin Pätzold, Martin Stergiopoulou, Katerina Goetz, Charlotte Ermakov, Vladimir Nikolaevich Shuvalov, Sergei Wild, James A. Blelly, Pierre Louis Mendillo, Michael Bertucci, Cesar Cartacci, Marco Orosei, Roberto Chu, Feng Kopf, Andrew J. Girazian, Zachary Roman, Michael T. |
author |
Sánchez Cano, Beatriz |
author_facet |
Sánchez Cano, Beatriz Lester, Mark Andrews, David J. Opgenoorth, Hermann Lillis, Robert Leblanc, François Fowler, Christopher M. Fang, Xiaohua Vaisberg, Oleg Mayyasi, Majd Holmberg, Mika Guo, Jingnan Hamrin, Maria Mazelle, Christian Peter, Kerstin Pätzold, Martin Stergiopoulou, Katerina Goetz, Charlotte Ermakov, Vladimir Nikolaevich Shuvalov, Sergei Wild, James A. Blelly, Pierre Louis Mendillo, Michael Bertucci, Cesar Cartacci, Marco Orosei, Roberto Chu, Feng Kopf, Andrew J. Girazian, Zachary Roman, Michael T. |
author_role |
author |
author2 |
Lester, Mark Andrews, David J. Opgenoorth, Hermann Lillis, Robert Leblanc, François Fowler, Christopher M. Fang, Xiaohua Vaisberg, Oleg Mayyasi, Majd Holmberg, Mika Guo, Jingnan Hamrin, Maria Mazelle, Christian Peter, Kerstin Pätzold, Martin Stergiopoulou, Katerina Goetz, Charlotte Ermakov, Vladimir Nikolaevich Shuvalov, Sergei Wild, James A. Blelly, Pierre Louis Mendillo, Michael Bertucci, Cesar Cartacci, Marco Orosei, Roberto Chu, Feng Kopf, Andrew J. Girazian, Zachary Roman, Michael T. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
COORDINATED MULTIPOINT MISSIONS ESA-VOYAGE2050 FUTURE MISSIONS MARS PLASMA SCIENCE GAPS |
topic |
COORDINATED MULTIPOINT MISSIONS ESA-VOYAGE2050 FUTURE MISSIONS MARS PLASMA SCIENCE GAPS |
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 objective of this White Paper, submitted to ESA’s Voyage 2050 call, is to get a more holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the undisturbed solar wind outside of the induced magnetosphere. This can only be achieved with coordinated multi-point observations with high temporal resolution as they have the scientific potential to track the whole dynamics of the system (from small to large scales), and they constitute the next generation of the exploration of Mars analogous to what happened at Earth a few decades ago. This White Paper discusses the key science questions that are still open at Mars and how they could be addressed with coordinated multipoint missions. The main science questions are: (i) How does solar wind driving impact the dynamics of the magnetosphere and ionosphere? (ii) What is the structure and nature of the tail of Mars’ magnetosphere at all scales? (iii) How does the lower atmosphere couple to the upper atmosphere? (iv) Why should we have a permanent in-situ Space Weather monitor at Mars? Each science question is devoted to a specific plasma region, and includes several specific scientific objectives to study in the coming decades. In addition, two mission concepts are also proposed based on coordinated multi-point science from a constellation of orbiting and ground-based platforms, which focus on understanding and solving the current science gaps. Fil: Sánchez Cano, Beatriz. University of Leicester; Reino Unido Fil: Lester, Mark. University of Leicester; Reino Unido Fil: Andrews, David J.. No especifíca; Fil: Opgenoorth, Hermann. Universidad de Umea; Suecia. University of Leicester; Reino Unido Fil: Lillis, Robert. No especifíca; Fil: Leblanc, François. Université Pierre et Marie Curie; Francia Fil: Fowler, Christopher M.. No especifíca; Fil: Fang, Xiaohua. State University of Colorado at Boulder; Estados Unidos Fil: Vaisberg, Oleg. Space Research Institute Of The Russian Academy Of Sciences; Rusia Fil: Mayyasi, Majd. Boston University; Estados Unidos Fil: Holmberg, Mika. No especifíca; Fil: Guo, Jingnan. Chinese Academy of Sciences; República de China Fil: Hamrin, Maria. Universidad de Umea; Suecia Fil: Mazelle, Christian. No especifíca; Fil: Peter, Kerstin. Universitat zu Köln; Alemania Fil: Pätzold, Martin. Universitat zu Köln; Alemania Fil: Stergiopoulou, Katerina. No especifíca; Fil: Goetz, Charlotte. No especifíca; Fil: Ermakov, Vladimir Nikolaevich. No especifíca; Fil: Shuvalov, Sergei. Space Research Institute Of The Russian Academy Of Sciences; Rusia Fil: Wild, James A.. Lancaster University; Reino Unido Fil: Blelly, Pierre Louis. No especifíca; Fil: Mendillo, Michael. Boston University; Estados Unidos 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: Cartacci, Marco. Istituto Nazionale di Astrofisica; Italia Fil: Orosei, Roberto. Istituto Di Radioastronomia; Italia Fil: Chu, Feng. University of Iowa; Estados Unidos Fil: Kopf, Andrew J.. No especifíca; Fil: Girazian, Zachary. University of Iowa; Estados Unidos Fil: Roman, Michael T.. University of Leicester; Reino Unido |
description |
The objective of this White Paper, submitted to ESA’s Voyage 2050 call, is to get a more holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the undisturbed solar wind outside of the induced magnetosphere. This can only be achieved with coordinated multi-point observations with high temporal resolution as they have the scientific potential to track the whole dynamics of the system (from small to large scales), and they constitute the next generation of the exploration of Mars analogous to what happened at Earth a few decades ago. This White Paper discusses the key science questions that are still open at Mars and how they could be addressed with coordinated multipoint missions. The main science questions are: (i) How does solar wind driving impact the dynamics of the magnetosphere and ionosphere? (ii) What is the structure and nature of the tail of Mars’ magnetosphere at all scales? (iii) How does the lower atmosphere couple to the upper atmosphere? (iv) Why should we have a permanent in-situ Space Weather monitor at Mars? Each science question is devoted to a specific plasma region, and includes several specific scientific objectives to study in the coming decades. In addition, two mission concepts are also proposed based on coordinated multi-point science from a constellation of orbiting and ground-based platforms, which focus on understanding and solving the current science gaps. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-11 |
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/11336/212538 Sánchez Cano, Beatriz; Lester, Mark; Andrews, David J.; Opgenoorth, Hermann; Lillis, Robert; et al.; Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation”; Springer; Experimental Astronomy; 54; 2-3; 11-2021; 641-676 0922-6435 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/212538 |
identifier_str_mv |
Sánchez Cano, Beatriz; Lester, Mark; Andrews, David J.; Opgenoorth, Hermann; Lillis, Robert; et al.; Mars’ plasma system: Scientific potential of coordinated multipoint missions: “The next generation”; Springer; Experimental Astronomy; 54; 2-3; 11-2021; 641-676 0922-6435 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-021-09790-0 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
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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1843606314702340096 |
score |
13.001348 |