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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZGivnK2Y/ShrBk
Repositóriosid.inpe.br/mtc-m17@80/2007/11.27.13.46
Última Atualização2010:09.24.19.42.28 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m17@80/2007/11.27.13.46.16
Última Atualização dos Metadados2018:06.05.03.35.32 (UTC) administrator
Chave SecundáriaINPE-14992-PRE/9903
ISSN0992-7689
Chave de CitaçãoKane:2007:HyLoCo
TítuloHysteresis loops of Cosmic Ray intensity decreases versus solar and interplanetary parameters
Ano2007
Data de Acesso25 jun. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho8260 KiB
2. Contextualização
AutorKane, Rajaram Purushottam
Identificador de Curriculo8JMKD3MGP5W/3C9JJ4U
GrupoDGE-INPE-MCT-BR
AfiliaçãoInstituto Nacional de Pesquisas Espaciais (INPE)
RevistaAnnales Geophysicae
Volume25
Número9
Páginas2087-2097
Histórico (UTC)2007-12-19 14:18:21 :: simone -> administrator ::
2008-06-29 02:37:37 :: administrator -> banon ::
2010-05-11 15:21:19 :: banon -> simone ::
2010-09-24 19:42:29 :: simone -> administrator ::
2012-10-24 00:03:42 :: administrator -> simone :: 2007
2013-02-20 15:20:08 :: simone -> marciana :: 2007
2013-03-07 13:47:37 :: marciana -> administrator :: 2007
2018-06-05 03:35:32 :: administrator -> marciana :: 2007
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-ChaveInterplanetary physics (Cosmic rays
Heliopause and solar wind termination
Interplanetary magnetic fields)
ResumoThe purpose of this study was to examine the correlation between CR (Cosmic Ray) intensity and solar, interplanetary and terrestrial parameters. The hysteresis loops of (CR) versus those of several solar parameters showed narrow loops in even cycles 20, 22 and broad loops in odd cycles 19, 21, as also in the recent odd cycle 23. Hysteresis plots for CR versus interplanetary number density N and speed V were erratic and uncertain (broad and narrow, all mixed up). Plots of CR versus Interplanetary magnetic field (IMF) B seemed to be narrow for even as well as odd cycles. Hysteresis loops between CR and other interplanetary parameters were not clear-cut. The same was true for terrestrial parameters. During sunspot maximum years 20002003 of cycle 23, there is a double peak structure in all parameters. Whereas CR have a peak spacing of 30 months, sunspots and Tilt angle have a spacing of only 20 months. The solar open magnetic flux and the Voyager 1 magnetic field have a spacing of 25 months. The solar polar magnetic field reverses later than the first peak of all parameters and hence, could not be a direct cause (as if effect started before the cause and lasted for several months more after the cause disappeared). It seems that CR modulation is mainly guided by magnetic configurations deep in the heliosphere, which may not have a simple relationship with parameters near Earth or near Sun.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Hysteresis loops of...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/6qtX3pFwXQZGivnK2Y/ShrBk
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZGivnK2Y/ShrBk
Idiomaen
Arquivo AlvoDr.kane-1.pdf
Grupo de Usuáriosadministrator
banon
marciana
simone
Visibilidadeshown
Detentor da CópiaSID/SCD
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 1
sid.inpe.br/mtc-m21/2012/07.13.14.58.38 1
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirolcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
e-Mail (login)marciana
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