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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZQjxQKY/GqbnS
Repositóriosid.inpe.br/ePrint@80/2005/06.10.14.42
Última Atualização2013:04.02.12.25.39 (UTC) administrator
Repositório de Metadadossid.inpe.br/ePrint@80/2005/06.10.14.42.47
Última Atualização dos Metadados2018:06.04.04.12.43 (UTC) administrator
Chave SecundáriaINPE--PRE/
ISSN0992-7689
Chave de CitaçãoRodriguesIHRKJRDT:2004:MuInSt
TítuloMulti-technique investigations of storm-time ionospheric irregularities over the São Luis equatorial station in Brazil
Ano2004
Data Secundária2004
Data de Acesso22 jun. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2158 KiB
2. Contextualização
Autor1 Rodrigues, Eurico de Paula.
2 Iyer, K. N.
3 Hysell, D. L.
4 Rodrigues, F. S.
5 Kherani, E. A.
6 Jardim, A. C.
7 Rezende, L. F. C.
8 Dutra, S. G.
9 Trivedi, Nalin Babulal
Grupo1 DGE-INPE-MCT-BR
2
3
4
5
6
7
8
9 DGE-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial(INPE,DGE)
2 Cornell Univ, Ithaca, NY 14853 USA
3 Saurashtra Univ, Dept Phys, Rajkot, Gujarat
RevistaAnnales Geophysicae
Volume22
Número10
Páginas3513-3522
Histórico (UTC)2008-04-18 15:26:31 :: alexandra -> banon ::
2009-07-14 21:35:11 :: banon -> administrator ::
2010-05-11 01:35:37 :: administrator -> banon ::
2010-05-11 15:20:51 :: banon -> alexandra ::
2010-05-14 01:58:01 :: alexandra -> administrator ::
2012-10-21 21:45:49 :: administrator -> marciana :: 2004
2013-03-07 14:19:33 :: marciana -> administrator :: 2004
2013-04-02 12:25:07 :: administrator -> marciana :: 2004
2013-04-02 12:25:39 :: marciana -> administrator :: 2004
2018-06-04 04:12:43 :: administrator -> marciana :: 2004
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-Chaveionosphere
ionospheric irregularities/GLOBAL POSITIONING SYSTEM
SPREAD-F
ELECTRIC-FIELDS
RADAR OBSERVATIONS
LOW-LATITUDE
MAGNETOSPHERIC DISTURBANCES
BACKSCATTER RADAR
GPS OBSERVATIONS
MAGNETIC STORMS
JULIA RADAR
ResumoOn 11 April 2001, a large magnetic storm occurred with SSC at 13:43 UT, and D-st reached below -200nT after two southward B-z excursions. The K-p index during this storm reached 8 and remained high (>4) for about 21 h, and the Sao Luis magnetometer H component presented simultaneous oscillations and decreased substantially relative to the previous magnetically quiet days. This storm triggered strong ionospheric irregularities, as observed by a recently installed 30 MHz coherent scatter radar, a digisonde, and a GPS scintillation receiver, all operating at the Sao Luis equatorial station (2.33degrees S, 44degrees W, dip latitude 1.3degrees S). The ionospheric conditions and the characteristics of the ionospheric irregularities observed by these instruments are presented and discussed. The VHF radar RTI (Range Time Intensity) echoes and their power spectra and spectral width for the storm night 11-12 April 2001, were used to analyse the nature and dynamics of the plasma irregularities and revealed the coexistence of many structures in the altitudinal range of 400-1200 km, some locally generated and others that drifted from other longitudinal sectors. The radar data also revealed that the plumes had periodic eastward and westward zonal velocities after 22:20 UT, when well-developed quiet-time plumes typically drift eastward. Another interesting new observation is that the F-layer remained anomalously high throughout the 11-12 April 2001 storm night (21:00 UT to 09:00 UT next day) (the LT at Sao Luis is UT -3 h), as indicated by the digisonde parameters hmF2 and h'F, which is a condition favourable for spread F generation and maintenance. The AE auroral index showed enhancements (followed by decreases) that are indicative of magnetospheric convection enhancements at about 15:00 UT, 20:00 UT and 22:00 UT on 11 April 2001 and at 00:20 UT (small amplitude) on 12 April 2001, associated with many B-z fluctuations, including clear two southward incursions that gave rise to large and long lasting K-p values and large negative D-st values. This intense auroral activity generated disturbance dynamo and prompt penetration electric fields that were responsible for the maintenance of the F-layer at a high altitude along the night of 11-12 April 2001. The short-lived F-region height rise seen between 16:00 to 18:00 UT on 11 April 2001 is probably due to the prompt penetration eastward electric fields of magnetospheric origin during the first IMF B-z turning to south around 15:00 UT.
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/6qtX3pFwXQZQjxQKY/GqbnS
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZQjxQKY/GqbnS
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Grupo de Usuáriosadministrator
alexandra
banon
marciana
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Edição Anteriorsid.inpe.br/yolanda/2004/12.15.11.11
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 1
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
7. Controle da descrição
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