Fechar

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3PJDGFL
Repositóriosid.inpe.br/mtc-m21b/2017/09.06.15.48   (acesso restrito)
Última Atualização2017:09.06.15.48.53 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21b/2017/09.06.15.48.53
Última Atualização dos Metadados2021:07.18.04.03.04 (UTC) administrator
DOI10.1016/j.jastp.2017.07.007
ISSN1364-6826
Chave de CitaçãoPietrellaPFJSKEC:2017:EqSpOc
TítuloEquinoctial spread-F occurrence at low latitudes in different longitude sectors under moderate and high solar activity
Ano2017
MêsNov.
Data de Acesso05 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho6012 KiB
2. Contextualização
Autor1 Pietrella, M.
2 Pezzopane, M.
3 Fagundes, P. R.
4 Jesus, Rodolfo de
5 Supnithi, P.
6 Klinngam, S.
7 Ezquer, R. G.
8 Cabrera, M. A.
Grupo1
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Istituto Nazionale di Geofisica e Vulcanologia
2 Istituto Nazionale di Geofisica e Vulcanologia
3 Universidade do Vale do Paraíba (UNIVAP)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 King Mongkut's Institute of Technology Ladkrabang (KMITL)
6 King Mongkut's Institute of Technology Ladkrabang (KMITL)
7 Universidad Tecnológica Nacional
8 Universidad Tecnológica Nacional
Endereço de e-Mail do Autor1 marco.pietrella@ingv.it
2
3
4 rodolfo.jesus@inpe.br
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Volume164
Páginas149-162
Nota SecundáriaA1_ENGENHARIAS_I A2_GEOCIÊNCIAS A2_ENGENHARIAS_III B1_INTERDISCIPLINAR B1_ENGENHARIAS_IV B1_BIODIVERSIDADE B2_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
Histórico (UTC)2017-09-06 15:48:53 :: simone -> administrator ::
2017-09-06 15:48:54 :: administrator -> simone :: 2017
2017-09-06 15:50:02 :: simone -> administrator :: 2017
2021-07-18 04:03:04 :: administrator -> simone :: 2017
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-ChaveIonosphereEquatorial ionosphereIonospheric irregularitiesWave propagation
ResumoA comparative study aimed to investigate the equatorial and low-latitude spread-F occurrences for moderate solar activity (MSA) and high solar activity (HSA), was carried out considering concurrent observations made in some ionospheric stations, which identify three separate longitudinal sectors: Chiang Mai (CGM; 18.8° N, 98.9° E, mag. Lat. 13.2° N) and Chumphon (CPN; 10.7° N, 99.4° E, mag. Lat. 3.2° N), Thailand; Palmas (PAL; 10.2° S, 311.8° E, mag. Lat. 0.9° S) and São José dos Campos (SJC; 23.2° S, 314.1° E, mag. Lat. 14.0° S), Brazil; Tucumán (TUC; 26.9° S, 294.6° E, mag. Lat. 16.8° S), Argentina. Spread-F phenomena recorded during the equinoctial months of September and October 2010, March and April 2011, for MSA, March and April 2014, September and October 2014, for HSA, were classified in two different modes: range spread-F (RSF) and frequency spread-F (FSF). The satellite trace (ST) occurrence was also investigated as possible precursor of spread-F events. When comparing the results of equatorial (CPN and PAL) and low-latitude (CGM, SJC, and TUC) stations, some common features independently of the solar activity emerge: (1) a prevalence of RSF signatures is observed in the time interval 20:0003:00 LT, while FSF occurrences prevail in the time interval 03:0006:00 LT; (2) STs are confirmed to be a possible precursor of RSF occurrences. For HSA, at equatorial latitudes, spread-F occurrences in the Thai sector (CPN) are higher than those observed in the Brazilian sector (PAL). When comparing the results of low-latitude stations of CGM, SJC, and TUC some unusual aspects characterizing the morphology of spread-F occurrences emerge: (1) contrary to the Thai and Argentine sectors, in the Brazilian sector (SJC), RSF and FSF appearances in September, for HSA, are observed with relatively long persistence times between about 03:00-06:00 LT and 01:00-03:00 LT respectively, while balanced RSF and FSF occurrences with short persistence times are observed for months for MSA; (2) a prevalence of FSF at CGM during the first half of September for MSA, never observed in the Brazilian and Argentine areas. During years of LSA and MSA common morphological aspects are found at CGM and SJC, that is a predominance of FSF, with the lowest persistence times characterizing SJC. This suggests that the low-latitude behaviour of spread-F occurrences, under different levels of solar activity, at least in the longitude sectors here analysed, can be to a some extent generalized.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Equinoctial spread-F occurrence...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 06/09/2017 12:48 1.0 KiB 
4. Condições de acesso e uso
Idiomaen
Arquivo Alvopietrella_equinoctial.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
Lista de Itens Citandosid.inpe.br/bibdigital/2013/09.29.20.43 1
DivulgaçãoWEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS.
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
e-Mail (login)simone
atualizar 


Fechar