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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/188288
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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) |
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CONICET Digital (CONICET) |
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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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1844614493661822976 |
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13.070432 |