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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/222463

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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling 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
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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