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Metadados

1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/4B639NB
Repositóriosid.inpe.br/mtc-m21d/2024/04.17.15.24
Repositório de Metadadossid.inpe.br/mtc-m21d/2024/04.17.15.24.38
Última Atualização dos Metadados2024:04.17.15.24.38 (UTC) simone
Chave SecundáriaINPE--PRE/
Chave de CitaçãoBravoSouMarVenBar:2024:EvIoIm
TítuloEvaluation of Ionospheric Impact Prediction during the Solar Eclipse of October 14, 2023
Ano2024
Data de Acesso19 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Bravo, Manuel
2 Souza, Jonas Rodrigues de
3 Martínez-Ledesma, Miguel
4 Venchiarutti, Valentín
5 Barbás, Blas de Haro
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHFE
Grupo1
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Universidad Adventista de Chile
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidad Adventista de Chile
4 Universidad Adventista de Chile
5 Universidad Adventista de Chile
Endereço de e-Mail do Autor1 manuelbravo@unach.cl
2 jonas.souza@inpe.br
Nome do EventoConferencia Latinoamericana de Geofísica Espacial, 14
Localização do EventoMonterrey, Mexico
Data08-12 Apr. 2024
Título do LivroProceedings
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
ResumoSolar eclipses are an excellent opportunity for ionospheric researchers to use as a natural ionospheric laboratory. The production of ions-electrons in the ionosphere is due to the photoionization process that depends directly on solar radiation. During a solar eclipse, the gradual decrease in solar radiation to totality (in some cases) creates a geographic window (minutes to hours) of nighttime conditions during daylight hours. Under these conditions it is possible to evaluate and study the response of some numerical models. The solar eclipse of October 14, 2023 was a partial solar eclipse that covered from North America, Central America and even northern part of South America. Prior to this event, predictions were made of the impact on the ionosphere during this eclipse. For this, the SUPIM (Sheffield University Plasmasphere-Ionosphere Model) was used: a numerical model that solves the coupled equations of continuity, momentum and energy dependent on time, along the magnetic field lines, and which has been updated and adapted by the Instituto Nacional de Pesquisas Espaciais (SUPIM-INPE). Particularly, in the case of predictions during solar eclipses, some adjustments have been made to the solar radiation according to the geometry of each solar eclipse. The objective of this work is to evaluate that prediction using the measurements available from some ionospheric stations that were covered during the eclipse. Modeling these phenomena helps us better understand the ionospheric impact and its consequences on communication and navigation systems.
ÁreaCEA
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4. Condições de acesso e uso
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Grupo de Usuáriossimone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
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6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark nextedition nexthigherunit notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url volume
7. Controle da descrição
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