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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3RD7J8L
Repositóriosid.inpe.br/mtc-m21c/2018/07.03.16.51   (acesso restrito)
Última Atualização2018:07.03.16.51.07 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2018/07.03.16.51.07
Última Atualização dos Metadados2020:12.07.21.11.57 (UTC) administrator
DOI10.1007/s11207-018-1303-8
ISSN0038-0938
1573-093X
Chave de CitaçãoAugustoNONRTMFSKS:2018:OnMaGe
TítuloThe 2015 summer solstice storm: one of the major geomagnetic storms of solar cycle 24 observed at ground level
Ano2018
Data de Acesso02 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho6344 KiB
2. Contextualização
Autor 1 Augusto, C. R. A.
 2 Navia, C. E.
 3 Oliveira, M. N. de
 4 Nepomuceno, A. A.
 5 Raulin, J. P.
 6 Tueros, E.
 7 Mendonça, Rafael Rodrigues Souza de
 8 Fauth, A. C.
 9 Souza, H. Vieira de
10 Kopenkin, V.
11 Sinzi, T.
Grupo 1
 2
 3
 4
 5
 6
 7 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação 1 Universidade Federal Fluminense (UFF)
 2 Universidade Federal Fluminense (UFF)
 3 Universidade Federal Fluminense (UFF)
 4 Universidade Federal Fluminense (UFF)
 5 Universidade Presbiteriana Mackenzie
 6 Universidade Presbiteriana Mackenzie
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Universidade Estadual de Campinas (UNICAMP)
 9 Universidade Estadual de Campinas (UNICAMP)
10 Waseda University
11 Rikkyo University
Endereço de e-Mail do Autor 1
 2
 3 paulista@fisica.if.uff.br
 4
 5
 6
 7 rafael.mendonca@inpe.br
RevistaSolar Physics
Volume293
Número5
Páginase84
Nota SecundáriaA2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_BIOTECNOLOGIA B1_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO
Histórico (UTC)2018-07-03 16:51:07 :: simone -> administrator ::
2018-07-03 16:51:08 :: administrator -> simone :: 2018
2018-07-03 16:53:05 :: simone -> administrator :: 2018
2020-12-07 21:11:57 :: administrator -> simone :: 2018
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-ChaveSun: activity · Astroparticle physics · Atmospheric effects · Instrumentation: detectors
ResumoWe report on the 22 23 June 2015 geomagnetic storm that occurred at the summer solstice. There have been fewer intense geomagnetic storms during the current solar cycle, Solar Cycle 24, than in the previous cycle. This situation changed after mid-June 2015, when one of the largest solar active regions (AR 12371) of Solar Cycle 24 that was located close to the central meridian, produced several coronal mass ejections (CMEs) associated with M-class flares. The impact of these CMEs on the Earths magnetosphere resulted in a moderate to severe G4-class geomagnetic storm on 22 23 June 2015 and a G2 (moderate) geomagnetic storm on 24 June. The G4 solstice storm was the second largest (so far) geomagnetic storm of Cycle 24. We highlight the ground-level observations made with the New-Tupi, Muonca, and the CARPET El Leoncito cosmic-ray detectors that are located within the South Atlantic Anomaly (SAA) region. These observations are studied in correlation with data obtained by space-borne detectors (ACE, GOES, SDO, and SOHO) and other ground-based experiments. The CME designations are taken from the Computer Aided CME Tracking (CACTus) automated catalog. As expected, Forbush decreases (FD) associated with the passing CMEs were recorded by these detectors. We note a peculiar feature linked to a severe geomagnetic storm event. The 21 June 2015 CME 0091 (CACTus CME catalog number) was likely associated with the 22 June summer solstice FD event. The angular width of CME 0091 was very narrow and measured ∼56∘ degrees seen from Earth. In most cases, only CME halos and partial halos lead to severe geomagnetic storms. We perform a cross-check analysis of the FD events detected during the rise phase of Solar Cycle 24, the geomagnetic parameters, and the CACTus CME catalog. Our study suggests that narrow angular-width CMEs that erupt in a westward direction from the SunEarth line can lead to moderate and severe geomagnetic storms. We also report on the strong solar proton radiation storm that began on 21 June. We did not find a signal from this SEP at ground level. The details of these observations are presented.
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4. Condições de acesso e uso
Idiomaen
Arquivo Alvoaugusto_2015.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentodenypublisher denyfinaldraft12
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 4
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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