Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites
Autor(a) principal: | |
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Data de Publicação: | 2015 |
Tipo de documento: | Tese |
Idioma: | eng |
Título da fonte: | Biblioteca Digital de Teses e Dissertações do INPE |
Texto Completo: | http://urlib.net/sid.inpe.br/mtc-m21b/2015/02.09.23.47 |
Resumo: | AB8TRACT: Magnetic reconnection is a fundamental plasma process defined as topological restructuring of magnetic fields due to changes in the connectivity of magnetic field lines. Although other phenomena, e.g., particle acceleration and heating, can happen concurrently associated with reconnection, it is the most important process because it allows the fast magnetic energy release in large scales. Flux transfer events (FTEs) are considered as a result of transient magnetic reconnection and are often observed in the vicinity of the Earth${'}$s magnetopause. Thus, the study on magnetic reconnection is one of the important issues for the solar wind-magnetospheric cou-pling processo The space physics community has been interested in FTEs since their discovery. Recently, computational simulations, and multi-point observations have provided advances to FTE generation and structure formation studies. In this work data collected by the THEMIS mission was used to investigate flux transfer events under multi-points observations, which allows to investigate the structure itself, how it influences external plasma dynamics and analyze their dynamics under magnetic reconnection location. Although the techniques presented here had been employed in previous studies, we believe that the analysis of equatorial FTEs using multipoint observations and of its subsequent motion have a big importance to better understand magnetic reconnection at the Earth${'}$s magnetopause. It was created a list of flux transfer events observed by THEMIS probes at the dayside of the magnetopause and characterized these events according to the solar wind parameters and magnetic reconnection locations. Also are presented case studies of FTEs observed at multi-point observations including representative signatures observed in dataset in this thesis. |
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info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesisStudy of flux transfer events observed at the Earth's magnetopause by THEMIS satellitesEstudo de eventos de transferência de fluxo observados na magnetopausa terrestre pelos satélites THEMIS2015-03-03Daiki KogaWalter Demetrio Gonzalez AlarconAlícia Luisa Clúa de Gonzalez AlarconRenato Sérgio DallaquaFernando Jaques Ruiz Simões JúniorFlávia Reis CardosoMarcos Vinicius Dias SilveiraInstituto Nacional de Pesquisas Espaciais (INPE)Programa de Pós-Graduação do INPE em Geofísica Espacial/Ciências do Ambiente Solar-TerrestreINPEBReventos de transferência de fluxoreconexão magnéticaeventos transientesmagnetopausamagnetosferaflux transfer eventsmagnetic field reconnectiontransient eventmagnetopausemagnetosphericAB8TRACT: Magnetic reconnection is a fundamental plasma process defined as topological restructuring of magnetic fields due to changes in the connectivity of magnetic field lines. Although other phenomena, e.g., particle acceleration and heating, can happen concurrently associated with reconnection, it is the most important process because it allows the fast magnetic energy release in large scales. Flux transfer events (FTEs) are considered as a result of transient magnetic reconnection and are often observed in the vicinity of the Earth${'}$s magnetopause. Thus, the study on magnetic reconnection is one of the important issues for the solar wind-magnetospheric cou-pling processo The space physics community has been interested in FTEs since their discovery. Recently, computational simulations, and multi-point observations have provided advances to FTE generation and structure formation studies. In this work data collected by the THEMIS mission was used to investigate flux transfer events under multi-points observations, which allows to investigate the structure itself, how it influences external plasma dynamics and analyze their dynamics under magnetic reconnection location. Although the techniques presented here had been employed in previous studies, we believe that the analysis of equatorial FTEs using multipoint observations and of its subsequent motion have a big importance to better understand magnetic reconnection at the Earth${'}$s magnetopause. It was created a list of flux transfer events observed by THEMIS probes at the dayside of the magnetopause and characterized these events according to the solar wind parameters and magnetic reconnection locations. Also are presented case studies of FTEs observed at multi-point observations including representative signatures observed in dataset in this thesis.Reconexão magnética é um processo fundemantal de plasma definido como uma reestruturação topológica do campo magnético devido à mudanças na conectividade das linhas do campo magnético. Embora fenômenos como aceleração e aquecimento de partículas também ocorram no plasma, a reconexão magnética é o mais importante pois permite a rápida conversão de energia magnética em grande escala. Eventos de transferência de fluxo são considerados o resultado da reconexão magnética transiente e são frequentemente observados na vizinhança da magnetopausa terrestre. Portanto, estudos sobre a reconexão magnética são tópicos muito importantes sobre o acoplamento do sistema vento solar-magnetosfera. A comunidade da geofísica espacial têm interesse sobre os FTEs desde a sua descoberta. Recentemente, a simulação computacional e multi-observação de satélites têm permitido avanços na pesquisa sobre modelos de geração e estrutura dos FTEs. Neste trabalho, usou-se dados obtidos pelos satélites da missão THEMIS para investigar os FTEs sob aspectos da reconexão magnética. Embora as técnicas apresentadas neste trabalho tenham sido empregadas em outros trabalhos, acredita-se que a análise de FTEs equatoriais através de multi-observações e o seu movimento subsequente sejam muito importantes para o entendimento da reconexão na magnetopausa terrestre. Portanto, foi analisada uma lista de FTEs no lado diurno da mangetopausa. Os eventos foram caracterizados de acordo com parâmetros do vento solar e de reconexão magnética.http://urlib.net/sid.inpe.br/mtc-m21b/2015/02.09.23.47info:eu-repo/semantics/openAccessengreponame:Biblioteca Digital de Teses e Dissertações do INPEinstname:Instituto Nacional de Pesquisas Espaciais (INPE)instacron:INPE2021-07-31T06:54:42Zoai:urlib.net:sid.inpe.br/mtc-m21b/2015/02.09.23.47.45-0Biblioteca Digital de Teses e Dissertaçõeshttp://bibdigital.sid.inpe.br/PUBhttp://bibdigital.sid.inpe.br/col/iconet.com.br/banon/2003/11.21.21.08/doc/oai.cgiopendoar:32772021-07-31 06:54:43.709Biblioteca Digital de Teses e Dissertações do INPE - Instituto Nacional de Pesquisas Espaciais (INPE)false |
dc.title.en.fl_str_mv |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
dc.title.alternative.pt.fl_str_mv |
Estudo de eventos de transferência de fluxo observados na magnetopausa terrestre pelos satélites THEMIS |
title |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
spellingShingle |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites Marcos Vinicius Dias Silveira |
title_short |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
title_full |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
title_fullStr |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
title_full_unstemmed |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
title_sort |
Study of flux transfer events observed at the Earth's magnetopause by THEMIS satellites |
author |
Marcos Vinicius Dias Silveira |
author_facet |
Marcos Vinicius Dias Silveira |
author_role |
author |
dc.contributor.advisor1.fl_str_mv |
Daiki Koga |
dc.contributor.advisor2.fl_str_mv |
Walter Demetrio Gonzalez Alarcon |
dc.contributor.referee1.fl_str_mv |
Alícia Luisa Clúa de Gonzalez Alarcon |
dc.contributor.referee2.fl_str_mv |
Renato Sérgio Dallaqua |
dc.contributor.referee3.fl_str_mv |
Fernando Jaques Ruiz Simões Júnior |
dc.contributor.referee4.fl_str_mv |
Flávia Reis Cardoso |
dc.contributor.author.fl_str_mv |
Marcos Vinicius Dias Silveira |
contributor_str_mv |
Daiki Koga Walter Demetrio Gonzalez Alarcon Alícia Luisa Clúa de Gonzalez Alarcon Renato Sérgio Dallaqua Fernando Jaques Ruiz Simões Júnior Flávia Reis Cardoso |
dc.description.abstract.por.fl_txt_mv |
AB8TRACT: Magnetic reconnection is a fundamental plasma process defined as topological restructuring of magnetic fields due to changes in the connectivity of magnetic field lines. Although other phenomena, e.g., particle acceleration and heating, can happen concurrently associated with reconnection, it is the most important process because it allows the fast magnetic energy release in large scales. Flux transfer events (FTEs) are considered as a result of transient magnetic reconnection and are often observed in the vicinity of the Earth${'}$s magnetopause. Thus, the study on magnetic reconnection is one of the important issues for the solar wind-magnetospheric cou-pling processo The space physics community has been interested in FTEs since their discovery. Recently, computational simulations, and multi-point observations have provided advances to FTE generation and structure formation studies. In this work data collected by the THEMIS mission was used to investigate flux transfer events under multi-points observations, which allows to investigate the structure itself, how it influences external plasma dynamics and analyze their dynamics under magnetic reconnection location. Although the techniques presented here had been employed in previous studies, we believe that the analysis of equatorial FTEs using multipoint observations and of its subsequent motion have a big importance to better understand magnetic reconnection at the Earth${'}$s magnetopause. It was created a list of flux transfer events observed by THEMIS probes at the dayside of the magnetopause and characterized these events according to the solar wind parameters and magnetic reconnection locations. Also are presented case studies of FTEs observed at multi-point observations including representative signatures observed in dataset in this thesis. Reconexão magnética é um processo fundemantal de plasma definido como uma reestruturação topológica do campo magnético devido à mudanças na conectividade das linhas do campo magnético. Embora fenômenos como aceleração e aquecimento de partículas também ocorram no plasma, a reconexão magnética é o mais importante pois permite a rápida conversão de energia magnética em grande escala. Eventos de transferência de fluxo são considerados o resultado da reconexão magnética transiente e são frequentemente observados na vizinhança da magnetopausa terrestre. Portanto, estudos sobre a reconexão magnética são tópicos muito importantes sobre o acoplamento do sistema vento solar-magnetosfera. A comunidade da geofísica espacial têm interesse sobre os FTEs desde a sua descoberta. Recentemente, a simulação computacional e multi-observação de satélites têm permitido avanços na pesquisa sobre modelos de geração e estrutura dos FTEs. Neste trabalho, usou-se dados obtidos pelos satélites da missão THEMIS para investigar os FTEs sob aspectos da reconexão magnética. Embora as técnicas apresentadas neste trabalho tenham sido empregadas em outros trabalhos, acredita-se que a análise de FTEs equatoriais através de multi-observações e o seu movimento subsequente sejam muito importantes para o entendimento da reconexão na magnetopausa terrestre. Portanto, foi analisada uma lista de FTEs no lado diurno da mangetopausa. Os eventos foram caracterizados de acordo com parâmetros do vento solar e de reconexão magnética. |
description |
AB8TRACT: Magnetic reconnection is a fundamental plasma process defined as topological restructuring of magnetic fields due to changes in the connectivity of magnetic field lines. Although other phenomena, e.g., particle acceleration and heating, can happen concurrently associated with reconnection, it is the most important process because it allows the fast magnetic energy release in large scales. Flux transfer events (FTEs) are considered as a result of transient magnetic reconnection and are often observed in the vicinity of the Earth${'}$s magnetopause. Thus, the study on magnetic reconnection is one of the important issues for the solar wind-magnetospheric cou-pling processo The space physics community has been interested in FTEs since their discovery. Recently, computational simulations, and multi-point observations have provided advances to FTE generation and structure formation studies. In this work data collected by the THEMIS mission was used to investigate flux transfer events under multi-points observations, which allows to investigate the structure itself, how it influences external plasma dynamics and analyze their dynamics under magnetic reconnection location. Although the techniques presented here had been employed in previous studies, we believe that the analysis of equatorial FTEs using multipoint observations and of its subsequent motion have a big importance to better understand magnetic reconnection at the Earth${'}$s magnetopause. It was created a list of flux transfer events observed by THEMIS probes at the dayside of the magnetopause and characterized these events according to the solar wind parameters and magnetic reconnection locations. Also are presented case studies of FTEs observed at multi-point observations including representative signatures observed in dataset in this thesis. |
publishDate |
2015 |
dc.date.issued.fl_str_mv |
2015-03-03 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/doctoralThesis |
status_str |
publishedVersion |
format |
doctoralThesis |
dc.identifier.uri.fl_str_mv |
http://urlib.net/sid.inpe.br/mtc-m21b/2015/02.09.23.47 |
url |
http://urlib.net/sid.inpe.br/mtc-m21b/2015/02.09.23.47 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
Instituto Nacional de Pesquisas Espaciais (INPE) |
dc.publisher.program.fl_str_mv |
Programa de Pós-Graduação do INPE em Geofísica Espacial/Ciências do Ambiente Solar-Terrestre |
dc.publisher.initials.fl_str_mv |
INPE |
dc.publisher.country.fl_str_mv |
BR |
publisher.none.fl_str_mv |
Instituto Nacional de Pesquisas Espaciais (INPE) |
dc.source.none.fl_str_mv |
reponame:Biblioteca Digital de Teses e Dissertações do INPE instname:Instituto Nacional de Pesquisas Espaciais (INPE) instacron:INPE |
reponame_str |
Biblioteca Digital de Teses e Dissertações do INPE |
collection |
Biblioteca Digital de Teses e Dissertações do INPE |
instname_str |
Instituto Nacional de Pesquisas Espaciais (INPE) |
instacron_str |
INPE |
institution |
INPE |
repository.name.fl_str_mv |
Biblioteca Digital de Teses e Dissertações do INPE - Instituto Nacional de Pesquisas Espaciais (INPE) |
repository.mail.fl_str_mv |
|
publisher_program_txtF_mv |
Programa de Pós-Graduação do INPE em Geofísica Espacial/Ciências do Ambiente Solar-Terrestre |
contributor_advisor1_txtF_mv |
Daiki Koga |
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1706809357377732608 |