Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November

Autores
Nieves Chinchilla, Teresa; Alzate, Nathalia; Cremades Fernandez, Maria Hebe; Rodríguez García, Laura; Santos, Luiz F. G. Dos; Narock, Ayris; Xie, Hong; Szabo, Adam; Palmerio, Erika; Krupar, Vratislav; Pulupa, Marc; Lario, David; Stevens, Michael L.; Wilson, Lynn B.; Kwon, Ryun Young; Mays, M. Leila; St. Cyr, O. Chris; Hess, Phillip; Reeves, Katharine K.; Seaton, Daniel B.; Niembro, Tatiana; Bale, Stuart D.; Kasper, Justin C.
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of the ICMEs were observed remotely at the Sun in EUV and subsequently tracked to their coronal counterparts in white light. This period is of particular interest to the community as it has been identified as the first widespread solar energetic particle event of solar cycle 25. The distribution of various solar and heliospheric-dedicated spacecraft throughout the inner heliosphere during PSP observations of these largescale magnetic structures enables a comprehensive analysis of the internal evolution and topology of such structures. By assembling different models and techniques, we identify the signatures of interaction between the two consecutive ICMEs and the implications for their internal structure. We use multispacecraft observations in combination with a remote-sensing forward modeling technique, numerical propagation models, and in situ reconstruction techniques. The outcome, from the full reconciliations, demonstrates that the two coronal mass ejections (CMEs) are interacting in the vicinity of the PSP. Thus, we identify the in situ observations based on the physical processes that are associated with the interaction and collision of both CMEs. We also expand the flux rope modeling and in situ reconstruction technique to incorporate the aging and expansion effects in a distorted internal magnetic structure and explore the implications of both effects in the magnetic configuration of the ICMEs.
Fil: Nieves Chinchilla, Teresa. National Aeronautics and Space Administration; Estados Unidos
Fil: Alzate, Nathalia. Adnet Systems, Inc.; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Cremades Fernandez, Maria Hebe. Universidad Tecnológica Nacional; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Rodríguez García, Laura. Universidad de Alcalá; España
Fil: Santos, Luiz F. G. Dos. State University of Colorado at Boulder; Estados Unidos
Fil: Narock, Ayris. Adnet Systems, Inc.; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Xie, Hong. Catholic University Of America; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Szabo, Adam. National Aeronautics and Space Administration; Estados Unidos
Fil: Palmerio, Erika. University of California; Estados Unidos
Fil: Krupar, Vratislav. National Aeronautics and Space Administration; Estados Unidos. University of Maryland; Estados Unidos
Fil: Pulupa, Marc. University of California at Berkeley; Estados Unidos
Fil: Lario, David. National Aeronautics and Space Administration; Estados Unidos
Fil: Stevens, Michael L.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Wilson, Lynn B.. National Aeronautics and Space Administration; Estados Unidos
Fil: Kwon, Ryun Young. Korea Astronomy And Space Science Institute; Corea del Sur
Fil: Mays, M. Leila. National Aeronautics and Space Administration; Estados Unidos
Fil: St. Cyr, O. Chris. National Aeronautics and Space Administration; Estados Unidos
Fil: Hess, Phillip. Spece Sciences División. Naval Research Laboratory; Estados Unidos
Fil: Reeves, Katharine K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Seaton, Daniel B.. State University of Colorado at Boulder; Estados Unidos. Space Science And Engineering Division; Estados Unidos
Fil: Niembro, Tatiana. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Bale, Stuart D.. University of California at Berkeley; Estados Unidos
Fil: Kasper, Justin C.. Bwx Technologies, Inc; Estados Unidos. University of Michigan; Estados Unidos
Materia
CORONAL MASS EJECTIONS
SOLAR WIND
INTERPLANETARY PHYSICS
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:11336/188288

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network_name_str CONICET Digital (CONICET)
spelling Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 NovemberNieves Chinchilla, TeresaAlzate, NathaliaCremades Fernandez, Maria HebeRodríguez García, LauraSantos, Luiz F. G. DosNarock, AyrisXie, HongSzabo, AdamPalmerio, ErikaKrupar, VratislavPulupa, MarcLario, DavidStevens, Michael L.Wilson, Lynn B.Kwon, Ryun YoungMays, M. LeilaSt. Cyr, O. ChrisHess, PhillipReeves, Katharine K.Seaton, Daniel B.Niembro, TatianaBale, Stuart D.Kasper, Justin C.CORONAL MASS EJECTIONSSOLAR WINDINTERPLANETARY PHYSICShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of the ICMEs were observed remotely at the Sun in EUV and subsequently tracked to their coronal counterparts in white light. This period is of particular interest to the community as it has been identified as the first widespread solar energetic particle event of solar cycle 25. The distribution of various solar and heliospheric-dedicated spacecraft throughout the inner heliosphere during PSP observations of these largescale magnetic structures enables a comprehensive analysis of the internal evolution and topology of such structures. By assembling different models and techniques, we identify the signatures of interaction between the two consecutive ICMEs and the implications for their internal structure. We use multispacecraft observations in combination with a remote-sensing forward modeling technique, numerical propagation models, and in situ reconstruction techniques. The outcome, from the full reconciliations, demonstrates that the two coronal mass ejections (CMEs) are interacting in the vicinity of the PSP. Thus, we identify the in situ observations based on the physical processes that are associated with the interaction and collision of both CMEs. We also expand the flux rope modeling and in situ reconstruction technique to incorporate the aging and expansion effects in a distorted internal magnetic structure and explore the implications of both effects in the magnetic configuration of the ICMEs.Fil: Nieves Chinchilla, Teresa. National Aeronautics and Space Administration; Estados UnidosFil: Alzate, Nathalia. Adnet Systems, Inc.; Estados Unidos. National Aeronautics and Space Administration; Estados UnidosFil: Cremades Fernandez, Maria Hebe. Universidad Tecnológica Nacional; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Rodríguez García, Laura. Universidad de Alcalá; EspañaFil: Santos, Luiz F. G. Dos. State University of Colorado at Boulder; Estados UnidosFil: Narock, Ayris. Adnet Systems, Inc.; Estados Unidos. National Aeronautics and Space Administration; Estados UnidosFil: Xie, Hong. Catholic University Of America; Estados Unidos. National Aeronautics and Space Administration; Estados UnidosFil: Szabo, Adam. National Aeronautics and Space Administration; Estados UnidosFil: Palmerio, Erika. University of California; Estados UnidosFil: Krupar, Vratislav. National Aeronautics and Space Administration; Estados Unidos. University of Maryland; Estados UnidosFil: Pulupa, Marc. University of California at Berkeley; Estados UnidosFil: Lario, David. National Aeronautics and Space Administration; Estados UnidosFil: Stevens, Michael L.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Wilson, Lynn B.. National Aeronautics and Space Administration; Estados UnidosFil: Kwon, Ryun Young. Korea Astronomy And Space Science Institute; Corea del SurFil: Mays, M. Leila. National Aeronautics and Space Administration; Estados UnidosFil: St. Cyr, O. Chris. National Aeronautics and Space Administration; Estados UnidosFil: Hess, Phillip. Spece Sciences División. Naval Research Laboratory; Estados UnidosFil: Reeves, Katharine K.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Seaton, Daniel B.. State University of Colorado at Boulder; Estados Unidos. Space Science And Engineering Division; Estados UnidosFil: Niembro, Tatiana. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Bale, Stuart D.. University of California at Berkeley; Estados UnidosFil: Kasper, Justin C.. Bwx Technologies, Inc; Estados Unidos. University of Michigan; Estados UnidosIOP Publishing2022-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/188288Nieves Chinchilla, Teresa; Alzate, Nathalia; Cremades Fernandez, Maria Hebe; Rodríguez García, Laura; Santos, Luiz F. G. Dos; et al.; Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November; IOP Publishing; Astrophysical Journal; 930; 1; 5-2022; 1-210004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ac590binfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac590binfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:45:24Zoai:ri.conicet.gov.ar:11336/188288instacron: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 10:45:25.087CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
title Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
spellingShingle Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
Nieves Chinchilla, Teresa
CORONAL MASS EJECTIONS
SOLAR WIND
INTERPLANETARY PHYSICS
title_short Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
title_full Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
title_fullStr Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
title_full_unstemmed Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
title_sort Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
dc.creator.none.fl_str_mv Nieves Chinchilla, Teresa
Alzate, Nathalia
Cremades Fernandez, Maria Hebe
Rodríguez García, Laura
Santos, Luiz F. G. Dos
Narock, Ayris
Xie, Hong
Szabo, Adam
Palmerio, Erika
Krupar, Vratislav
Pulupa, Marc
Lario, David
Stevens, Michael L.
Wilson, Lynn B.
Kwon, Ryun Young
Mays, M. Leila
St. Cyr, O. Chris
Hess, Phillip
Reeves, Katharine K.
Seaton, Daniel B.
Niembro, Tatiana
Bale, Stuart D.
Kasper, Justin C.
author Nieves Chinchilla, Teresa
author_facet Nieves Chinchilla, Teresa
Alzate, Nathalia
Cremades Fernandez, Maria Hebe
Rodríguez García, Laura
Santos, Luiz F. G. Dos
Narock, Ayris
Xie, Hong
Szabo, Adam
Palmerio, Erika
Krupar, Vratislav
Pulupa, Marc
Lario, David
Stevens, Michael L.
Wilson, Lynn B.
Kwon, Ryun Young
Mays, M. Leila
St. Cyr, O. Chris
Hess, Phillip
Reeves, Katharine K.
Seaton, Daniel B.
Niembro, Tatiana
Bale, Stuart D.
Kasper, Justin C.
author_role author
author2 Alzate, Nathalia
Cremades Fernandez, Maria Hebe
Rodríguez García, Laura
Santos, Luiz F. G. Dos
Narock, Ayris
Xie, Hong
Szabo, Adam
Palmerio, Erika
Krupar, Vratislav
Pulupa, Marc
Lario, David
Stevens, Michael L.
Wilson, Lynn B.
Kwon, Ryun Young
Mays, M. Leila
St. Cyr, O. Chris
Hess, Phillip
Reeves, Katharine K.
Seaton, Daniel B.
Niembro, Tatiana
Bale, Stuart D.
Kasper, Justin C.
author2_role 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
SOLAR WIND
INTERPLANETARY PHYSICS
topic CORONAL MASS EJECTIONS
SOLAR WIND
INTERPLANETARY PHYSICS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of the ICMEs were observed remotely at the Sun in EUV and subsequently tracked to their coronal counterparts in white light. This period is of particular interest to the community as it has been identified as the first widespread solar energetic particle event of solar cycle 25. The distribution of various solar and heliospheric-dedicated spacecraft throughout the inner heliosphere during PSP observations of these largescale magnetic structures enables a comprehensive analysis of the internal evolution and topology of such structures. By assembling different models and techniques, we identify the signatures of interaction between the two consecutive ICMEs and the implications for their internal structure. We use multispacecraft observations in combination with a remote-sensing forward modeling technique, numerical propagation models, and in situ reconstruction techniques. The outcome, from the full reconciliations, demonstrates that the two coronal mass ejections (CMEs) are interacting in the vicinity of the PSP. Thus, we identify the in situ observations based on the physical processes that are associated with the interaction and collision of both CMEs. We also expand the flux rope modeling and in situ reconstruction technique to incorporate the aging and expansion effects in a distorted internal magnetic structure and explore the implications of both effects in the magnetic configuration of the ICMEs.
Fil: Nieves Chinchilla, Teresa. National Aeronautics and Space Administration; Estados Unidos
Fil: Alzate, Nathalia. Adnet Systems, Inc.; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Cremades Fernandez, Maria Hebe. Universidad Tecnológica Nacional; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Rodríguez García, Laura. Universidad de Alcalá; España
Fil: Santos, Luiz F. G. Dos. State University of Colorado at Boulder; Estados Unidos
Fil: Narock, Ayris. Adnet Systems, Inc.; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Xie, Hong. Catholic University Of America; Estados Unidos. National Aeronautics and Space Administration; Estados Unidos
Fil: Szabo, Adam. National Aeronautics and Space Administration; Estados Unidos
Fil: Palmerio, Erika. University of California; Estados Unidos
Fil: Krupar, Vratislav. National Aeronautics and Space Administration; Estados Unidos. University of Maryland; Estados Unidos
Fil: Pulupa, Marc. University of California at Berkeley; Estados Unidos
Fil: Lario, David. National Aeronautics and Space Administration; Estados Unidos
Fil: Stevens, Michael L.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Wilson, Lynn B.. National Aeronautics and Space Administration; Estados Unidos
Fil: Kwon, Ryun Young. Korea Astronomy And Space Science Institute; Corea del Sur
Fil: Mays, M. Leila. National Aeronautics and Space Administration; Estados Unidos
Fil: St. Cyr, O. Chris. National Aeronautics and Space Administration; Estados Unidos
Fil: Hess, Phillip. Spece Sciences División. Naval Research Laboratory; Estados Unidos
Fil: Reeves, Katharine K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Seaton, Daniel B.. State University of Colorado at Boulder; Estados Unidos. Space Science And Engineering Division; Estados Unidos
Fil: Niembro, Tatiana. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Bale, Stuart D.. University of California at Berkeley; Estados Unidos
Fil: Kasper, Justin C.. Bwx Technologies, Inc; Estados Unidos. University of Michigan; Estados Unidos
description We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of the ICMEs were observed remotely at the Sun in EUV and subsequently tracked to their coronal counterparts in white light. This period is of particular interest to the community as it has been identified as the first widespread solar energetic particle event of solar cycle 25. The distribution of various solar and heliospheric-dedicated spacecraft throughout the inner heliosphere during PSP observations of these largescale magnetic structures enables a comprehensive analysis of the internal evolution and topology of such structures. By assembling different models and techniques, we identify the signatures of interaction between the two consecutive ICMEs and the implications for their internal structure. We use multispacecraft observations in combination with a remote-sensing forward modeling technique, numerical propagation models, and in situ reconstruction techniques. The outcome, from the full reconciliations, demonstrates that the two coronal mass ejections (CMEs) are interacting in the vicinity of the PSP. Thus, we identify the in situ observations based on the physical processes that are associated with the interaction and collision of both CMEs. We also expand the flux rope modeling and in situ reconstruction technique to incorporate the aging and expansion effects in a distorted internal magnetic structure and explore the implications of both effects in the magnetic configuration of the ICMEs.
publishDate 2022
dc.date.none.fl_str_mv 2022-05
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/11336/188288
Nieves Chinchilla, Teresa; Alzate, Nathalia; Cremades Fernandez, Maria Hebe; Rodríguez García, Laura; Santos, Luiz F. G. Dos; et al.; Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November; IOP Publishing; Astrophysical Journal; 930; 1; 5-2022; 1-21
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/188288
identifier_str_mv Nieves Chinchilla, Teresa; Alzate, Nathalia; Cremades Fernandez, Maria Hebe; Rodríguez García, Laura; Santos, Luiz F. G. Dos; et al.; Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November; IOP Publishing; Astrophysical Journal; 930; 1; 5-2022; 1-21
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ac590b
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac590b
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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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