Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter
- Autores
- Mierla, Marilena; Cremades Fernandez, Maria Hebe; Andretta, Vincenzo; Chifu, Iulia; Zhukov, Andrei N.; Susino, Roberto; Auchère, Frédéric; Vourlidas, Angelos; Talpeanu, Dana Camelia; Rodriguez, Luciano; Janssens, Jan; Nicula, Bogdan; Aznar Cuadrado, Regina; Berghmans, David; Bemporad, Alessandro; D’Huys, Elke; Dolla, Laurent; Gissot, Samuel; Jerse, Giovanna; Kraaikamp, Emil; Long, David M.; Mampaey, Benjamin; Möstl, Christian; Pagano, Paolo; Parenti, Susanna; West, Matthew J.; Podladchikova, Olena; Romoli, Marco; Sasso, Clementina; Stegen, Koen; Teriaca, Luca; Thompson, William; Verbeeck, Cis; Davies, Emma
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- On February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions were associated with coronal mass ejections (CMEs) observed by Metis, Solar Orbiter’s coronagraph. All three eruptions were also observed by instruments onboard the Solar–TErrestrial RElations Observatory (Ahead; STEREO-A), the Solar Dynamics Observatory (SDO), and the Solar and Heliospheric Observatory (SOHO). Here we present an analysis of these eruptions. We investigate their morphology, direction of propagation, and 3D properties. We demonstrate the success of applying two 3D reconstruction methods to three CMEs and their corresponding prominences observed from three perspectives and different distances from the Sun. This allows us to analyze the evolution of the events, from the erupting prominences low in the corona to the corresponding CMEs high in the corona. We also study the changes in the global magnetic field before and after the eruptions and the magnetic field configuration at the site of the eruptions using magnetic field extrapolation methods. This work highlights the importance of multi-perspective observations in studying the morphology of the erupting prominences, their source regions, and associated CMEs. The upcoming Solar Orbiter observations from higher latitudes will help to constrain this kind of study better.
Fil: Mierla, Marilena. Royal Observatory Of Belgium (rob);
Fil: Cremades Fernandez, Maria Hebe. Universidad de Mendoza. Facultad de Ingenieria; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Andretta, Vincenzo. Istituto Nazionale di Astrofisica; Italia
Fil: Chifu, Iulia. Universität Göttingen; Alemania
Fil: Zhukov, Andrei N.. Royal Observatory Of Belgium (rob);
Fil: Susino, Roberto. Istituto Nazionale di Astrofisica; Italia
Fil: Auchère, Frédéric. Universite Paris-saclay (universite Paris-saclay);
Fil: Vourlidas, Angelos. University Johns Hopkins; Estados Unidos
Fil: Talpeanu, Dana Camelia. Royal Observatory Of Belgium (rob);
Fil: Rodriguez, Luciano. Royal Observatory Of Belgium (rob);
Fil: Janssens, Jan. Royal Observatory Of Belgium (rob);
Fil: Nicula, Bogdan. Royal Observatory Of Belgium (rob);
Fil: Aznar Cuadrado, Regina. Max-Planck-Institut für Sonnensystemforschung; Alemania
Fil: Berghmans, David. Royal Observatory Of Belgium (rob);
Fil: Bemporad, Alessandro. Istituto Nazionale di Astrofisica; Italia
Fil: D’Huys, Elke. Royal Observatory Of Belgium (rob);
Fil: Dolla, Laurent. Royal Observatory Of Belgium (rob);
Fil: Gissot, Samuel. Royal Observatory Of Belgium (rob);
Fil: Jerse, Giovanna. Royal Observatory Of Belgium (rob);
Fil: Kraaikamp, Emil. Royal Observatory Of Belgium (rob);
Fil: Long, David M.. The Queens University of Belfast; Irlanda
Fil: Mampaey, Benjamin. Royal Observatory Of Belgium (rob);
Fil: Möstl, Christian. Austrian Space Weather Office; Austria
Fil: Pagano, Paolo. Università degli Studi di Palermo; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Parenti, Susanna. Universite Paris-saclay (universite Paris-saclay);
Fil: West, Matthew J.. Southwest Research Institute.; Estados Unidos
Fil: Podladchikova, Olena. National Polytechnic University of Ukraine; Ucrania. Leibniz Institute for Astrophysics Potsdam; Alemania
Fil: Romoli, Marco. Università di Firenze; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Sasso, Clementina. Istituto Nazionale di Astrofisica; Italia
Fil: Stegen, Koen. Royal Observatory Of Belgium (rob);
Fil: Teriaca, Luca. Max-Planck-Institut für Sonnensystemforschung; Alemania
Fil: Thompson, William. National Aeronautics and Space Administration; Estados Unidos
Fil: Verbeeck, Cis. Royal Observatory Of Belgium (rob);
Fil: Davies, Emma. University of New Hampshire; Estados Unidos - Materia
-
CORONAL MASS EJECTIONS
CORONAL MASS EJECTIONS
DYNAMICS
INITIATION AND PROPAGATION
LOW CORONAL SIGNATURES
PROMINENCES - 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:11336/222463
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Three Eruptions Observed by Remote Sensing Instruments Onboard Solar OrbiterMierla, MarilenaCremades Fernandez, Maria HebeAndretta, VincenzoChifu, IuliaZhukov, Andrei N.Susino, RobertoAuchère, FrédéricVourlidas, AngelosTalpeanu, Dana CameliaRodriguez, LucianoJanssens, JanNicula, BogdanAznar Cuadrado, ReginaBerghmans, DavidBemporad, AlessandroD’Huys, ElkeDolla, LaurentGissot, SamuelJerse, GiovannaKraaikamp, EmilLong, David M.Mampaey, BenjaminMöstl, ChristianPagano, PaoloParenti, SusannaWest, Matthew J.Podladchikova, OlenaRomoli, MarcoSasso, ClementinaStegen, KoenTeriaca, LucaThompson, WilliamVerbeeck, CisDavies, EmmaCORONAL MASS EJECTIONSCORONAL MASS EJECTIONSDYNAMICSINITIATION AND PROPAGATIONLOW CORONAL SIGNATURESPROMINENCEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1On February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions were associated with coronal mass ejections (CMEs) observed by Metis, Solar Orbiter’s coronagraph. All three eruptions were also observed by instruments onboard the Solar–TErrestrial RElations Observatory (Ahead; STEREO-A), the Solar Dynamics Observatory (SDO), and the Solar and Heliospheric Observatory (SOHO). Here we present an analysis of these eruptions. We investigate their morphology, direction of propagation, and 3D properties. We demonstrate the success of applying two 3D reconstruction methods to three CMEs and their corresponding prominences observed from three perspectives and different distances from the Sun. This allows us to analyze the evolution of the events, from the erupting prominences low in the corona to the corresponding CMEs high in the corona. We also study the changes in the global magnetic field before and after the eruptions and the magnetic field configuration at the site of the eruptions using magnetic field extrapolation methods. This work highlights the importance of multi-perspective observations in studying the morphology of the erupting prominences, their source regions, and associated CMEs. The upcoming Solar Orbiter observations from higher latitudes will help to constrain this kind of study better.Fil: Mierla, Marilena. Royal Observatory Of Belgium (rob);Fil: Cremades Fernandez, Maria Hebe. Universidad de Mendoza. Facultad de Ingenieria; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Andretta, Vincenzo. Istituto Nazionale di Astrofisica; ItaliaFil: Chifu, Iulia. Universität Göttingen; AlemaniaFil: Zhukov, Andrei N.. Royal Observatory Of Belgium (rob);Fil: Susino, Roberto. Istituto Nazionale di Astrofisica; ItaliaFil: Auchère, Frédéric. Universite Paris-saclay (universite Paris-saclay);Fil: Vourlidas, Angelos. University Johns Hopkins; Estados UnidosFil: Talpeanu, Dana Camelia. Royal Observatory Of Belgium (rob);Fil: Rodriguez, Luciano. Royal Observatory Of Belgium (rob);Fil: Janssens, Jan. Royal Observatory Of Belgium (rob);Fil: Nicula, Bogdan. Royal Observatory Of Belgium (rob);Fil: Aznar Cuadrado, Regina. Max-Planck-Institut für Sonnensystemforschung; AlemaniaFil: Berghmans, David. Royal Observatory Of Belgium (rob);Fil: Bemporad, Alessandro. Istituto Nazionale di Astrofisica; ItaliaFil: D’Huys, Elke. Royal Observatory Of Belgium (rob);Fil: Dolla, Laurent. Royal Observatory Of Belgium (rob);Fil: Gissot, Samuel. Royal Observatory Of Belgium (rob);Fil: Jerse, Giovanna. Royal Observatory Of Belgium (rob);Fil: Kraaikamp, Emil. Royal Observatory Of Belgium (rob);Fil: Long, David M.. The Queens University of Belfast; IrlandaFil: Mampaey, Benjamin. Royal Observatory Of Belgium (rob);Fil: Möstl, Christian. Austrian Space Weather Office; AustriaFil: Pagano, Paolo. Università degli Studi di Palermo; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Parenti, Susanna. Universite Paris-saclay (universite Paris-saclay);Fil: West, Matthew J.. Southwest Research Institute.; Estados UnidosFil: Podladchikova, Olena. National Polytechnic University of Ukraine; Ucrania. Leibniz Institute for Astrophysics Potsdam; AlemaniaFil: Romoli, Marco. Università di Firenze; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Sasso, Clementina. Istituto Nazionale di Astrofisica; ItaliaFil: Stegen, Koen. Royal Observatory Of Belgium (rob);Fil: Teriaca, Luca. Max-Planck-Institut für Sonnensystemforschung; AlemaniaFil: Thompson, William. National Aeronautics and Space Administration; Estados UnidosFil: Verbeeck, Cis. Royal Observatory Of Belgium (rob);Fil: Davies, Emma. University of New Hampshire; Estados UnidosSpringer2023-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/222463Mierla, Marilena; Cremades Fernandez, Maria Hebe; Andretta, Vincenzo; Chifu, Iulia; Zhukov, Andrei N.; et al.; Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter; Springer; Solar Physics; 298; 3; 3-2023; 1-300038-0938CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/10.1007/s11207-023-02137-2info:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-023-02137-2info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:00:17Zoai:ri.conicet.gov.ar:11336/222463instacron: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 10:00:18.094CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
title |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
spellingShingle |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter Mierla, Marilena CORONAL MASS EJECTIONS CORONAL MASS EJECTIONS DYNAMICS INITIATION AND PROPAGATION LOW CORONAL SIGNATURES PROMINENCES |
title_short |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
title_full |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
title_fullStr |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
title_full_unstemmed |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
title_sort |
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter |
dc.creator.none.fl_str_mv |
Mierla, Marilena Cremades Fernandez, Maria Hebe Andretta, Vincenzo Chifu, Iulia Zhukov, Andrei N. Susino, Roberto Auchère, Frédéric Vourlidas, Angelos Talpeanu, Dana Camelia Rodriguez, Luciano Janssens, Jan Nicula, Bogdan Aznar Cuadrado, Regina Berghmans, David Bemporad, Alessandro D’Huys, Elke Dolla, Laurent Gissot, Samuel Jerse, Giovanna Kraaikamp, Emil Long, David M. Mampaey, Benjamin Möstl, Christian Pagano, Paolo Parenti, Susanna West, Matthew J. Podladchikova, Olena Romoli, Marco Sasso, Clementina Stegen, Koen Teriaca, Luca Thompson, William Verbeeck, Cis Davies, Emma |
author |
Mierla, Marilena |
author_facet |
Mierla, Marilena Cremades Fernandez, Maria Hebe Andretta, Vincenzo Chifu, Iulia Zhukov, Andrei N. Susino, Roberto Auchère, Frédéric Vourlidas, Angelos Talpeanu, Dana Camelia Rodriguez, Luciano Janssens, Jan Nicula, Bogdan Aznar Cuadrado, Regina Berghmans, David Bemporad, Alessandro D’Huys, Elke Dolla, Laurent Gissot, Samuel Jerse, Giovanna Kraaikamp, Emil Long, David M. Mampaey, Benjamin Möstl, Christian Pagano, Paolo Parenti, Susanna West, Matthew J. Podladchikova, Olena Romoli, Marco Sasso, Clementina Stegen, Koen Teriaca, Luca Thompson, William Verbeeck, Cis Davies, Emma |
author_role |
author |
author2 |
Cremades Fernandez, Maria Hebe Andretta, Vincenzo Chifu, Iulia Zhukov, Andrei N. Susino, Roberto Auchère, Frédéric Vourlidas, Angelos Talpeanu, Dana Camelia Rodriguez, Luciano Janssens, Jan Nicula, Bogdan Aznar Cuadrado, Regina Berghmans, David Bemporad, Alessandro D’Huys, Elke Dolla, Laurent Gissot, Samuel Jerse, Giovanna Kraaikamp, Emil Long, David M. Mampaey, Benjamin Möstl, Christian Pagano, Paolo Parenti, Susanna West, Matthew J. Podladchikova, Olena Romoli, Marco Sasso, Clementina Stegen, Koen Teriaca, Luca Thompson, William Verbeeck, Cis Davies, Emma |
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 author author author author |
dc.subject.none.fl_str_mv |
CORONAL MASS EJECTIONS CORONAL MASS EJECTIONS DYNAMICS INITIATION AND PROPAGATION LOW CORONAL SIGNATURES PROMINENCES |
topic |
CORONAL MASS EJECTIONS CORONAL MASS EJECTIONS DYNAMICS INITIATION AND PROPAGATION LOW CORONAL SIGNATURES PROMINENCES |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
On February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions were associated with coronal mass ejections (CMEs) observed by Metis, Solar Orbiter’s coronagraph. All three eruptions were also observed by instruments onboard the Solar–TErrestrial RElations Observatory (Ahead; STEREO-A), the Solar Dynamics Observatory (SDO), and the Solar and Heliospheric Observatory (SOHO). Here we present an analysis of these eruptions. We investigate their morphology, direction of propagation, and 3D properties. We demonstrate the success of applying two 3D reconstruction methods to three CMEs and their corresponding prominences observed from three perspectives and different distances from the Sun. This allows us to analyze the evolution of the events, from the erupting prominences low in the corona to the corresponding CMEs high in the corona. We also study the changes in the global magnetic field before and after the eruptions and the magnetic field configuration at the site of the eruptions using magnetic field extrapolation methods. This work highlights the importance of multi-perspective observations in studying the morphology of the erupting prominences, their source regions, and associated CMEs. The upcoming Solar Orbiter observations from higher latitudes will help to constrain this kind of study better. Fil: Mierla, Marilena. Royal Observatory Of Belgium (rob); Fil: Cremades Fernandez, Maria Hebe. Universidad de Mendoza. Facultad de Ingenieria; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Andretta, Vincenzo. Istituto Nazionale di Astrofisica; Italia Fil: Chifu, Iulia. Universität Göttingen; Alemania Fil: Zhukov, Andrei N.. Royal Observatory Of Belgium (rob); Fil: Susino, Roberto. Istituto Nazionale di Astrofisica; Italia Fil: Auchère, Frédéric. Universite Paris-saclay (universite Paris-saclay); Fil: Vourlidas, Angelos. University Johns Hopkins; Estados Unidos Fil: Talpeanu, Dana Camelia. Royal Observatory Of Belgium (rob); Fil: Rodriguez, Luciano. Royal Observatory Of Belgium (rob); Fil: Janssens, Jan. Royal Observatory Of Belgium (rob); Fil: Nicula, Bogdan. Royal Observatory Of Belgium (rob); Fil: Aznar Cuadrado, Regina. Max-Planck-Institut für Sonnensystemforschung; Alemania Fil: Berghmans, David. Royal Observatory Of Belgium (rob); Fil: Bemporad, Alessandro. Istituto Nazionale di Astrofisica; Italia Fil: D’Huys, Elke. Royal Observatory Of Belgium (rob); Fil: Dolla, Laurent. Royal Observatory Of Belgium (rob); Fil: Gissot, Samuel. Royal Observatory Of Belgium (rob); Fil: Jerse, Giovanna. Royal Observatory Of Belgium (rob); Fil: Kraaikamp, Emil. Royal Observatory Of Belgium (rob); Fil: Long, David M.. The Queens University of Belfast; Irlanda Fil: Mampaey, Benjamin. Royal Observatory Of Belgium (rob); Fil: Möstl, Christian. Austrian Space Weather Office; Austria Fil: Pagano, Paolo. Università degli Studi di Palermo; Italia. Istituto Nazionale di Astrofisica; Italia Fil: Parenti, Susanna. Universite Paris-saclay (universite Paris-saclay); Fil: West, Matthew J.. Southwest Research Institute.; Estados Unidos Fil: Podladchikova, Olena. National Polytechnic University of Ukraine; Ucrania. Leibniz Institute for Astrophysics Potsdam; Alemania Fil: Romoli, Marco. Università di Firenze; Italia. Istituto Nazionale di Astrofisica; Italia Fil: Sasso, Clementina. Istituto Nazionale di Astrofisica; Italia Fil: Stegen, Koen. Royal Observatory Of Belgium (rob); Fil: Teriaca, Luca. Max-Planck-Institut für Sonnensystemforschung; Alemania Fil: Thompson, William. National Aeronautics and Space Administration; Estados Unidos Fil: Verbeeck, Cis. Royal Observatory Of Belgium (rob); Fil: Davies, Emma. University of New Hampshire; Estados Unidos |
description |
On February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions were associated with coronal mass ejections (CMEs) observed by Metis, Solar Orbiter’s coronagraph. All three eruptions were also observed by instruments onboard the Solar–TErrestrial RElations Observatory (Ahead; STEREO-A), the Solar Dynamics Observatory (SDO), and the Solar and Heliospheric Observatory (SOHO). Here we present an analysis of these eruptions. We investigate their morphology, direction of propagation, and 3D properties. We demonstrate the success of applying two 3D reconstruction methods to three CMEs and their corresponding prominences observed from three perspectives and different distances from the Sun. This allows us to analyze the evolution of the events, from the erupting prominences low in the corona to the corresponding CMEs high in the corona. We also study the changes in the global magnetic field before and after the eruptions and the magnetic field configuration at the site of the eruptions using magnetic field extrapolation methods. This work highlights the importance of multi-perspective observations in studying the morphology of the erupting prominences, their source regions, and associated CMEs. The upcoming Solar Orbiter observations from higher latitudes will help to constrain this kind of study better. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-03 |
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/11336/222463 Mierla, Marilena; Cremades Fernandez, Maria Hebe; Andretta, Vincenzo; Chifu, Iulia; Zhukov, Andrei N.; et al.; Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter; Springer; Solar Physics; 298; 3; 3-2023; 1-30 0038-0938 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/222463 |
identifier_str_mv |
Mierla, Marilena; Cremades Fernandez, Maria Hebe; Andretta, Vincenzo; Chifu, Iulia; Zhukov, Andrei N.; et al.; Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter; Springer; Solar Physics; 298; 3; 3-2023; 1-30 0038-0938 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://link.springer.com/10.1007/s11207-023-02137-2 info:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-023-02137-2 |
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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |