Fechar

1. Identificação
Tipo de ReferênciaCapítulo de Livro (Book Section)
Sitemtc-m16.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGPDW/3PBE3C2
Repositóriosid.inpe.br/mtc-m16/2017/07.25.17.15   (acesso restrito)
Última Atualização2017:07.25.17.15.14 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m16/2017/07.25.17.15.14
Última Atualização dos Metadados2023:12.29.17.40.43 (UTC) simone
Chave SecundáriaINPE--/
ISBN978-0-87590-432-0
Chave de CitaçãoGuarnieri:2006:1920
TítuloThe Nature of auroras during High-Intensity Long-Duration Continuous AE Activity (HILDCAA) events: 1998 to 200
Ano2006
Data de Acesso04 maio 2024
Tipo SecundárioPRE LI
Número de Arquivos1
Tamanho1001 KiB
2. Contextualização
AutorGuarnieri, Fernando Luis
GrupoDGE-INPE-MCT-BR
AfiliaçãoInstituto Nacional de Pesquisas Espaciais (INPE)
EditorTsurutani, B. T.
McPherron, R.
Gonzalez Alarcon, W. D.
Lu, G.
Sobra, J. H. A.
Título do LivroRecurrente magnetic storms: corotating solar wind streams
Editora (Publisher)AGU
CidadeWashington
Páginas235-243
Título da SérieGeophysical monograph 167
Histórico (UTC)2017-07-25 17:15:14 :: simone -> administrator ::
2023-12-29 17:40:00 :: administrator -> simone :: 2006
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-ChaveAuroras
HILDCAA
ResumoThe nature of auroras during High-Intensity Long-Duration Continuous AE Activity (HILDCAA) events occurred from 1998 to 2001 is studied using auroral images in Lyman-Birge-Hopfield Long (LBHL - 160 to 180 nm) wavelengths taken by the UVI instrument onboard the POLAR satellite. It is found that during HILDCAA events, auroras are occurring not only in the midnight sector, but at all local times along the auroral oval. During some events, auroras are noted even over the polar cap as well. The typical auroral intensities observed during HILDCAA events are in the range from 30 to 60 photon cm−2 s−1. Using a method to evaluate relative photon fluxes based on POLAR images, the photon fluxes during HILDCAAs were qualitatively compared with those during magnetic storm main and recovery phases. It is found that, for the auroral zone midnight sector, the relative photon fluxes during the main phases of storms are much higher than those during HILDCAA intervals, as expected. However, photon fluxes observed during HILDCAA events are generally higher than that during the recovery phase of storms. Thus, if integrated over long periods of time (a year), the energy input from particle precipitation into the ionosphere during the declining phase/ minimum phase of the solar cycle, when HILDCAAs/corotating solar wind streams dominate, could be greater than during solar maximum, when interplanetary coronal mass ejections (ICMEs) predominate. This is in agreement with several parallel studies based on the AE and Dst indices that indicate similar conclusions.
ÁreaCEA
ArranjoThe Nature of...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 25/07/2017 14:15 1.8 KiB 
4. Condições de acesso e uso
Idiomaen
Arquivo Alvoguarnieri.pdf
Grupo de Usuáriosadministrator
simone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 1
DivulgaçãoNTRSNASA; BNDEPOSITOLEGAL.
Acervo Hospedeirosid.inpe.br/banon/2003/08.15.17.40
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress edition electronicmailaddress format issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype translator url volume
7. Controle da descrição
e-Mail (login)simone
atualizar 


Fechar