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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3TKKK2H
Repositóriosid.inpe.br/mtc-m21c/2019/07.10.11.58
Repositório de Metadadossid.inpe.br/mtc-m21c/2019/07.10.11.58.05
Última Atualização dos Metadados2020:01.06.11.42.16 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoBatistaSaSoAbBrBa:2019:MoLoLa
TítuloModelling the low latitude ionosphere response to magnetic disturbances
Ano2019
Data de Acesso02 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Batista, Inez Staciarini
2 Santos, A. M.
3 Souza, Jonas Rodrigues de
4 Abdu, Mangalathayil Ali
5 Bravo, M.
6 Bailey, G.
Identificador de Curriculo1 8JMKD3MGP5W/3C9JHDA
2
3 8JMKD3MGP5W/3C9JHFE
4 8JMKD3MGP5W/3C9JHNK
Grupo1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
2
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Universidad de Concepción
6 Sheffield University
Endereço de e-Mail do Autor1 inez.batista@inpe.br
2
3 jonas.souza@inpe.br
4 ma.abdu@inpe.br
Nome do EventoIUGG General Assembly, 27
Localização do EventoMontréal, Canada
Data08-18 July
Histórico (UTC)2019-07-10 11:58:06 :: simone -> administrator ::
2020-01-06 11:42:16 :: administrator -> simone :: 2019
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoThe space weather events originated in the Sun can affect the whole thermosphere-ionosphere system at all latitudes. During such events disturbance electric fields (undershielding or overshielding) can penetrate from high to low latitudes causing significant disturbances in the electron density distribution and in the equatorial ionization anomaly (EIA) development. Besides that, the large amount of energy deposited in the polar region during disturbed periods will be responsible for the generation of disturbed winds that will flow towards the equator where they produce a disturbance dynamo which also affects the EIA density distribution. The TIDs and TADs are also sources of disturbances that propagate at high velocity reaching the equator 2-3 hours after the beginning of the magnetic storm. Particle precipitation is an additional source of perturbation at high latitudes as well as at the South Atlantic Magnetic Anomaly, where the conductivity can be affected by the extra ionization. Modeling the ionosphere during such disturbed periods is one of the most challenging tasks due to the complexity of the phenomena that affect the thermosphere environment as a whole. In this work we use the Sheffield University Plasmasphere-Ionosphere Model at INPE (SUPIM-INPE), to simulate the effects that were observed at the low latitude ionosphere in the South America longitude sector during some magnetic storm event. For some storms a few models are tested for the disturbed electric field and for the disturbed wind. A particle precipitation model is included in SUPIM, in order to test the ionospheric response to the enhanced conductivity.
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4. Condições de acesso e uso
Grupo de Usuáriossimone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark mirrorrepository nextedition 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 versiontype volume
7. Controle da descrição
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