Resultado da Pesquisa
A expressão de busca foi <related:sid.inpe.br/plutao/2014/06.03.22.53.24-0:en:title:2:geomagnetic interplanetary activity interval:interplanetary causes geomagnetic activity during 7 17 march 2012 interval cawses ii overview:>.
12 referências similares foram encontradas(inclusive a original) buscando em 17 dentre 17 Arquivos
(este total pode incluir algumas duplicatas - para ver a conta certa clique no botão Mostrar Todas).
As 10 mais recentes estão listadas abaixo.
Data e hora local de busca: 19/04/2024 06:33.

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W/3GDQQT5
Repositóriosid.inpe.br/plutao/2014/06.03.22.53   (acesso restrito)
Última Atualização2014:07.17.16.39.45 (UTC) administrator
Repositório de Metadadossid.inpe.br/plutao/2014/06.03.22.53.24
Última Atualização dos Metadados2018:06.04.23.39.32 (UTC) administrator
DOI10.1051/swsc/2013056
ISSN2115-7251
Rótulolattes: 3368023405805386 6 TsurutaniESVMGKP:2014:CAIIOv
Chave de CitaçãoTsurutaniESVMGKP:2014:CAIIOv
TítuloThe interplanetary causes of geomagnetic activity during the 7-17 March 2012 interval: a CAWSES II overview
Ano2014
Data de Acesso19 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1315 KiB
2. Contextualização
Autor1 Tsurutani, Bruce T.
2 Echer, Ezequiel
3 Shibata, Kazunari
4 Verkhoglyadova, Olga P.
5 Mannucci, Anthony J.
6 Gonzalez, Walter Demetrio
7 Kozyra, Janet U.
8 Pätzold, Martin
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JH3D
3
4
5
6 8JMKD3MGP5W/3C9JJC4
Grupo1
2 DGE-CEA-INPE-MCTI-GOV-BR
3
4
5
6 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3
4
5
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2 eecher@dge.inpe.br
Endereço de e-Mailmarcelo.pazos@inpe.br
RevistaJournal of Space Weather and Space Climate
Volume4
PáginasA02
Nota SecundáriaB5_GEOCIÊNCIAS
Histórico (UTC)2014-06-03 22:53:24 :: lattes -> administrator ::
2018-06-04 23:39:32 :: administrator -> marcelo.pazos@inpe.br :: 2014
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-ChaveAtividade Geomagnetica
Geomagnetic storms
ÁreaCEA
ArranjoFonds > Produção anterior à 2021 > DIDGE > The interplanetary causes...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Arquivo AlvoTsurutani_2014swscCAWSESII.pdf
Grupo de Usuáriosadministrator
lattes
marcelo.pazos@inpe.br
self-uploading-INPE-MCTI-GOV-BR
Grupo de Leitoresadministrator
marcelo.pazos@inpe.br
Visibilidadeshown
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhoiconet.com.br/banon/2006/11.26.21.31
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.15.01.50 2
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
NotasSetores de Atividade: Pesquisa e desenvolvimento científico.
Campos Vaziosabstract alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
e-Mail (login)marcelo.pazos@inpe.br
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemarte3.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YCT/GUif2
Repositóriosid.inpe.br/iris@1905/2005/07.29.01.58.39   (acesso restrito)
Última Atualização2015:09.08.15.55.59 (UTC) marciana
Repositório de Metadadossid.inpe.br/iris@1905/2005/07.29.01.59
Última Atualização dos Metadados2018:06.06.04.14.25 (UTC) administrator
Chave SecundáriaINPE-5818-PRE/1964
ISSN0032-0633
Rótulo7199
Chave de CitaçãoTsurutaniGoSmGoTaAkAn:1990:InSoCa
TítuloThe interplanetary and solar causes of geomagnetic activity
Ano1990
Data Secundária19960104
Data de Acesso19 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1505 KiB
2. Contextualização
Autor1 Tsurutani, Bruce T.
2 Goldstein, Bruce E.
3 Smith, Edward J.
4 Gonzalez-Alarcon, Walter Demetrio
5 Tang, Frances
6 Akasofu, Syun I.
7 Anderson, Roger R
Grupo1 DGE-INPE-BR
RevistaPlanetary and Space Science
Volume38
Número1
Páginas109-126
Histórico (UTC)2014-09-29 15:13:34 :: administrator -> marciana :: 1990
2015-09-08 15:55:59 :: marciana -> administrator :: 1990
2018-06-06 04:14:25 :: administrator -> marciana :: 1990
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveGEOFISICA ESPACIAL
ResumoWe present a review of recent work done on the topic of interplanetary and solar causes of geomagnetic activity. During solar maximum (1978-1979), 90 of the major magnetic storms (Dst <- 100 nT) are caused by large southward Bz events associated with interplanetary shocks. Of these, roughly half of the Bz events are located in the sheath and half associated with the driver gas. These two sources of southward IMFs often give magnetic storms a two-step profile. The sheath field events are generated in the interplanetary medium between the outer corona and the Earth from the "shocking" of the slow solar wind upstream of the high speed stream. In constrast, the driver gas events are fields which come from the solar source region. A correlation between the field orientation at the solar source and that at 1 a.u. was sought, but none was found. Thus, quantitative predictions of storm intensities from solar observations appear to be very difficult. Prominence eruptions are shown to be an important cause of the high speed solar wind streams that lead to magnetic storms. The other 10 of the major magnetic storms (Dst <- 100 nT) are caused by large southward Bz events associated with interplanetary shocks. Of these, roughly half of the Bz events are located in the sheath and half associated with the driver gas. These two sources of southward IMFs often give magnetic storms a two-step profile. The sheath field events are generated in the interplanetary medium between the outer corona and the Earth from the "shocking" of the slow solar wind upstream of the high speed stream. In constrast, the driver gas events are fields which come from the solar source region. A correlation between the field orientation at the solar source and that at 1 a.u. was sought, but none was found. Thus, quantitative predictions of storm intensities from solar observations appear to be very difficult. Prominence eruptions are shown to be an important cause of the high speed solar wind streams that lead to magnetic storms. The other 10 of the magnetic storms are not related to interplanetary shocks or high speed streams, but to high density "non-compressional density enhancements". Following magnetic storms are "high density long duration AE activity events"(HILDCAAs) that are series of continuous auroral substorms that last from days to weeks during of after the storm's recovery phase HILDCAAs can also occur independently of magnetic storms. This continuous auroral activity is caused by the southward component of the magnetic field of interplanetary Alfven waves, presumably through the process of magnetic reconnection with the Earth's field. These Alfven wave trains are often observed in the trailing portions of high speed streams. From an analysis of a year's data during solar maximum, it is found that the interplanetary medium is "Alfvenic" approx. 60 of the time. There appear to be no substantial differences in magnetopheric response to Alfvenic or non-Alfvenic interplanetary intervals. The magnetopause boundary layer is shown to contain broad-band ELF/VLF plasma waves at least 85 of the time at all dayside local times. These waves have sufficient amplitude to cause cross-field diffusion of magnetosheath plasma to form the low latitude boundary layer. Pitch angle scattering of the low latitude boundary layer particles is adequate to account for the dayside aurora. The only interplanetary/magnetosheath parameter that appears to affect the wave intensities is the IMF Bz. Although the waves are present at almost all times, they are intensified during southward IMF Bz intervals.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The interplanetary and...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Arquivo Alvo1990_tsurutani.pdf
Grupo de Usuáriosadministrator
marciana
Grupo de Leitoresadministrator
marciana
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/3EU29DP
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2001/04.03.15.36
6. Notas
Campos Vaziosaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
e-Mail (login)marciana
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemarte3.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YCT/GUJvv
Repositóriosid.inpe.br/iris@1905/2005/07.29.21.42.47
Última Atualização2017:12.01.15.35.16 (UTC) marciana
Repositório de Metadadossid.inpe.br/iris@1905/2005/07.29.21.42.54
Última Atualização dos Metadados2018:06.06.04.03.42 (UTC) administrator
Chave SecundáriaINPE-7316-PRE/3211
ISSN0148-0227
2156-2202
Rótulo8647
Chave de CitaçãoTsurutaniGoGoTaAr:1995:InOrGe
TítuloInterplanetary origin of geomagnetic activity in the declining phase of the solar cycle
Ano1995
Data Secundária20000106
MêsNov.
Data de Acesso19 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho854 KiB
2. Contextualização
Autor1 Tsurutani, Bruce T.
2 Gonzalez-Alarcon, Walter Demetrio
3 Gonzalez, Alicia Luisa Clua
4 Tang, Frances
5 Arballo, John K.
6 okada, Masaki
Grupo1 DGE-INPE-MCT-BR
RevistaJournal of Geophysical Research
Volume100
NúmeroA11
Páginas21717-21733
Histórico (UTC)2014-09-29 15:13:40 :: administrator -> marciana :: 1995
2017-12-01 15:35:16 :: marciana -> administrator :: 1995
2018-06-06 04:03:42 :: administrator -> marciana :: 1995
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveGEOFISICA ESPACIAL
MAGNETOSFERA
TEMPESTADES MAGNETICAS
CICLO SOLAR
ResumoInterplanetary magnetic field (IMF) and plasma data are compared with ground-based geomagnetic Dst and AE indices to determine the causes of magnetic storms, substorms, and quiet during the descending phase of the solar cycle. In this paper we focus primarily on 1974 when the AE index is anomalously high (AE = 283 nT). This year is characterized by the presence of two long-lasting corotating streams associated with coronal holes. The corotating streams interact with the upstream low-velocity (300-350 km s-1), high-density heliospheric current sheet (HCS) plasma sheet, which leads to field compression and 15 to 25-nT hourly average values. Although the Bz component in this corotating interaction region (CIR) is often < - 10 nT, typically the field directionality is highly variable, and large southward components have durations less than 3 hours. Thus the corotating strean/HCS plasma sheet interaction region can cause recurring moderate (-100 nT:5 Dst... -50 nT) to weak (50 nT...Dst:5 -25 nT) storms, and sometimes no significant ring current activity at all (Dst > -25 nT). Storms of major (Dst... - 100 nT) intensities were not associated with CIRs. Solar wind energy is transferred to the magnetosphere via magnetic reconnection during the weak and moderate storms. Because the B, component in the interaction region is typically highly fluctuating, the corresponding storm main phase profile is highly irregular. Reverse shocks are sometimes present at the sunward edge of the CIR. Because these events cause sharp decreases in field magnitude, they can be responsible for storm recovery phase onsets. The initial phases of these corotating stream-related storms are caused by the increased ram pressure associated with the HCS plasma sheet and the further density enhancement from the stream-stream compression. Although the solar wind speed is generally low in this region of space, the densities can be well over an order of magnitude higher than the average value, leading to significant positive Dst values. Since there are typically no forward shocks at 1 AU associated with the stream-stream interactions, the initial phases have gradual onsets. The most dramatic geomagnetic response to the corotating streams are chains of consecutive substorms caused by the southward components of large-amplitude Alfven waves within the body of the corotating streams. This auroral activity has been previously named high-intensity long-duration continuous AE activity (HILDCAAs). The substorm activity is generally most intense near the peak speed of the stream where the Alfven wave amplitudes are greatest, and it decreases with decreasing wave amplitudes and stream speed. Each of the 27-day recurring HILDCAA events can last 10 days or more, and the presence of two events per solar rotation is the cause of the exceptionally high AE average for 1974 (higher than 1979). HILDCAAs often occur during the recovery phase of magnetic storms, and the fresh (and sporadic) injection of substorin energy leads to unusually long storm recovery phases as noted in Dst In the far trailing edge of the corotating stream, the IMF amplitudes become low, <3 nT, and there is an absence of large-amplitude fluctuations (Alfven waves). This is related to and causes geomagnetic quiet. There were three major (Dst... -100 nT) storms that occurred in 1974. Each was caused by a nonrecurring moderate speed stream led by a fast forward shock. The mechanisms for generating the intense interplanetary B, which were responsible for the subsequent intense magnetic storms was shock compression of preexisting southwardly directed Bz (Bs) for the two largest events and a magnetic cloud for the third (weakest) event. Each of the three streams occurred near a HCS crossing with no obvious solar optical or X ray signatures. It is speculated that these events may be associated with flux openings associated with coronal hole expansions. In conclusion, we present a model of geomagnetic activity during the descending phase of the solar cycle. It incorporates storm initial phases, main phases, HILDCAAs, and geomagnetic quiet. It uses some of the recent Ulysses results. We feel that this model is sufficiently developed that it may be used for predictions, and we encourage testing during the current Dhase of the solar cycle.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Interplanetary origin 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/6qtX3pFwXQZ3r59YCT/GUJvv
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZ3r59YCT/GUJvv
Arquivo Alvo7316.pdf
Grupo de Usuáriosadministrator
Grupo de Leitoresadministrator
marciana
Visibilidadeshown
Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2001/04.03.15.36
6. Notas
Campos Vaziosaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
e-Mail (login)marciana
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YDa/Jsbnf
Repositóriosid.inpe.br/iris@1916/2005/12.13.17.00   (acesso restrito)
Última Atualização2014:04.29.17.58.05 (UTC) administrator
Repositório de Metadadossid.inpe.br/iris@1916/2005/12.13.17.00.27
Última Atualização dos Metadados2018:06.05.01.16.23 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1016/j.asr.2003.04.076
ISSN0273-1177
Chave de CitaçãoEcherGoDaViGuGoSc:2005:InShGe
TítuloInterplanetary shocks and geomagnetic activity during solar maximum (2000) and solar minimum (1995-1996)
ProjetoFAPESP (projects 98/04732-4 and 98/15959-0)
Ano2005
Data de Acesso19 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho141 KiB
2. Contextualização
Autor1 Echer, Ezequiel
2 Gonzalez, Walter Demetrio
3 Dal Lago, Alisson
4 Vieira, Luis Eduardo Antunes
5 Guarnieri, F. L.
6 Gonzalez, Alicia Luisa Clua de
7 Schuch, Nelson Jorge
Grupo1 DGE-INPE-MCT-BR
2 DGE-INPE-MCT-BR
3 DGE-INPE-MCT-BR
4 DGE-INPE-MCT-BR
5
6 DGE-INPE-MCT-BR
7 RSU-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 eecher@dge.inpe.br
2 gonzalez@dge.inpe.br
3 alisson.dallago@inpe.br
4 luis.vieira@inpe.br
5
6 alicia.gonzalez@inpe.br
7 njschuch@lacesm.ufsm.br
RevistaAdvances in Space Research
Volume36
Número12
Páginas2318-2322
Histórico (UTC)2006-07-27 15:52:09 :: simone -> administrator ::
2010-05-11 20:14:00 :: administrator -> simone ::
2012-10-03 14:43:06 :: simone -> administrator ::
2014-04-29 17:40:45 :: administrator -> marciana :: 2005
2014-04-29 17:58:08 :: marciana -> administrator :: 2005
2018-06-05 01:16:23 :: administrator -> :: 2005
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 shocks
geomagnetic activity
solar maximum
coronal mass ejections
magnetic storms
parameters
ResumoPlasma and magnetic field parameter variations through fast forward interplanetary shocks were correlated with the peak geomagnetic activity index Dst in a period from 0 to 3 days after the shock, during solar maximum (2000) and solar minimum (1995-1996). Solar wind speed (V) and total magnetic field (B-t) were the parameters with higher correlations with peak Dst index. The correlation coefficients were higher during solar minimum (r(2) = 56% for V and 39% for B-t) than during solar maximum (r(2) = 15% for V and 12% for B-t). A statistical distribution of geomagnetic activity levels following interplanetary shocks was obtained. It was observed that during solar maximum, 36% and 28% of interplanetary shocks were followed by intense (Dst <= - 100 nT) and moderate (-50 <= Dst < - 100 nT) geomagnetic activity, whereas during solar minimum 13% and 33% of the shocks were followed by intense and moderate geomagnetic activity. It can be concluded that the upstream/downstream variations of V and B-t through the shocks were the parameters better correlated with geomagnetic activity level, and during solar maximum a higher relative number of interplanetary shocks can be followed by intense geomagnetic activity than during solar minimum. One can extrapolate, for forecasting goals, that during a whole solar cycle a shock has a probability of around 50% to be followed by intense/moderate geomagnetic activity.
ÁreaCEA
Arranjo 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Interplanetary shocks and...
Arranjo 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Interplanetary shocks and...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Arquivo Alvo1-s2.0-S0273117705004527-main.pdf
Grupo de Usuáriosadministrator
simone
Grupo de Leitoresadministrator
marciana
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/3EU29DP
8JMKD3MGPCW/3EUFCFP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 1
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2003/08.15.17.40
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 resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/39RSEC2
Repositóriodpi.inpe.br/plutao/2011/06.11.14.29.51
Última Atualização2011:07.25.17.27.22 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2011/06.11.14.29.52
Última Atualização dos Metadados2018:06.05.00.01.21 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.5194/angeo-29-839-2011
ISSN0992-7689
Rótulolattes: 3368023405805386 3 TsurutaniEcheGonz:2011:CoMiSm
Chave de CitaçãoTsurutaniEcheGonz:2011:CoMiSm
TítuloThe solar and interplanetary causes of the recent minimum in geomagnetic activity (MGA23): a combination of midlatitude small coronal holes, low IMF <I>B</I><sub>Z</sub> variances, low solar wind speeds and low solar magnetic fields
ProjetoCNPq agency PQ-300211/2008-2 FAPESP agency 2007/52533-1 2008/06650-9
Ano2011
Data de Acesso19 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2057 KiB
2. Contextualização
Autor1 Tsurutani, B. T.
2 Echer, Ezequiel
3 Gonzalez, Walter Demetrio
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JH3D
Grupo1
2 DGE-CEA-INPE-MCT-BR
3 DGE-CEA-INPE-MCT-BR
Afiliação1 CALTECH, Jet Prop Lab, Pasadena, CA USA
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2
3 gonzalez@dge.inpe.br
Endereço de e-Mailgonzalez@dge.inpe.br
RevistaAnnales Geophysicae
Volume29
Número5
Páginas839-849
Histórico (UTC)2011-06-11 17:43:48 :: lattes -> administrator :: 2011
2011-07-25 17:20:01 :: administrator -> marciana :: 2011
2011-07-25 17:27:22 :: marciana -> administrator :: 2011
2011-07-25 21:25:41 :: administrator -> marciana :: 2011
2011-08-04 14:41:00 :: marciana -> administrator :: 2011
2011-11-09 20:22:57 :: administrator -> marciana :: 2011
2011-11-10 12:59:55 :: marciana -> banon :: 2011
2011-11-23 13:37:42 :: banon -> tereza@sid.inpe.br :: 2011
2011-11-25 13:58:24 :: tereza@sid.inpe.br -> administrator :: 2011
2018-06-05 00:01:21 :: administrator -> tereza@sid.inpe.br :: 2011
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-ChaveMagnetospheric physics
Solar wind-magnetosphere interactions
ORIGIN
STORMS
CYCLE
ResumoMinima in geomagnetic activity (MGA) at Earth at the ends of SC23 and SC22 have been identified. The two MGAs (called MGA23 and MGA22, respectively) were present in 2009 and 1997, delayed from the sunspot number minima in 2008 and 1996 by similar to 1/2-1 years. Part of the solar and interplanetary causes of the MGAs were exceptionally low solar (and thus low interplanetary) magnetic fields. Another important factor in MGA23 was the disappearance of equatorial and low latitude coronal holes and the appearance of midlatitude coronal holes. The location of the holes relative to the ecliptic plane led to low solar wind speeds and low IMF (B(z)) variances (sigma(2)(Bz)) and normalized variances (sigma(2)(Bz)/B(0)(2)) at Earth, with concomitant reduced solar wind-magnetospheric energy coupling. One result was the lowest ap indices in the history of ap recording. The results presented here are used to comment on the possible solar and interplanetary causes of the low geomagnetic activity that occurred during the Maunder Minimum.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The solar and...
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/J8LNKAN8RW/39RSEC2
URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/39RSEC2
Idiomaen
Arquivo Alvoangeo-29-839-2011.pdf
Grupo de Usuáriosadministrator
banon
lattes
marciana
tereza@sid.inpe.br
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
e-Mail (login)tereza@sid.inpe.br
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/4935EFS
Repositóriosid.inpe.br/mtc-m21d/2023/05.03.12.49   (acesso restrito)
Última Atualização2023:05.03.12.49.30 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21d/2023/05.03.12.49.30
Última Atualização dos Metadados2024:01.02.17.16.42 (UTC) administrator
DOI10.1007/s13538-023-01294-w
ISSN0103-9733
Chave de CitaçãoEcherLuHaFrBoNa:2023:GeAcFo
TítuloGeomagnetic Activity Following Interplanetary Shocks in Solar Cycles 23 and 24
Ano2023
MêsJune
Data de Acesso19 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PN
Número de Arquivos1
Tamanho3293 KiB
2. Contextualização
Autor1 Echer, Ezequiel
2 Lucas, Aline de
3 Hajra, Rajkumar
4 Franco, Adriane Marques de Souza
5 Bolzan, Mauricio J. A.
6 Nascimento, Luis Eduardo Sales do
Identificador de Curriculo1 8JMKD3MGP5W/3C9JH3D
ORCID1 0000-0002-8351-6779
Grupo1 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Federal de Educacao, Ciencia e Tecnologia de São Paulo (IFSP)
3 Indian Institute of Technology Indore
4 Universidade Federal do Sul e Sudeste do Pará
5 Universidade Federal de Jatai
6 Instituto Federal de Educacao, Ciencia e Tecnologia de São Paulo (IFSP)
Endereço de e-Mail do Autor1 ezequiel.echer@gmail.com
RevistaBrazilian Journal of Physics
Volume53
Número3
Páginase79
Nota SecundáriaB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_CIÊNCIAS_AGRÁRIAS_I B1_BIODIVERSIDADE B1_ASTRONOMIA_/_FÍSICA B2_ODONTOLOGIA B2_MATERIAIS B2_FARMÁCIA B2_ENGENHARIAS_II B2_ECONOMIA B2_CIÊNCIA_DA_COMPUTAÇÃO B3_MEDICINA_II B3_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B3_CIÊNCIAS_AMBIENTAIS B3_BIOTECNOLOGIA B4_QUÍMICA B4_ENSINO B4_CIÊNCIAS_BIOLÓGICAS_III B4_CIÊNCIAS_BIOLÓGICAS_II B4_CIÊNCIAS_BIOLÓGICAS_I
Histórico (UTC)2023-05-03 12:49:31 :: simone -> administrator ::
2023-05-03 12:49:31 :: administrator -> simone :: 2023
2023-05-03 12:50:22 :: simone -> administrator :: 2023
2024-01-02 17:16:42 :: administrator -> simone :: 2023
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-ChaveCoronal mass ejections
Geomagnetic disturbances
Magnetic reconnection
Magnetosphere
Shock waves
Solar cycle
Solar wind
ResumoInterplanetary shocks are important precursors of interplanetary coronal mass ejections (ICMEs) and corotating interaction regions (CIRs). The shock compression and draping effects on the interplanetary magnetic field (IMF) in sheaths can lead to significant geomagnetic activity. We identified 297 fast forward shocks observed by the Advanced Composition Explorer spacecraft upstream of the Earth, and analyzed their geomagnetic impacts in solar cycle (SC) 23 (19982008) and SC24 (20092018). The shock (normalized) occurrence rate is found to be significantly higher during SC23 compared to SC24, and it exhibits a stronger correlation with the sunspot number during SC23 (correlation coefficient r= 0.93) than during SC24 (r= 0.86). The average shock compressions of the IMF magnitude and plasma density are ≈ 2.0 and ≈ 2.4 , respectively, with no significant correlation with geomagnetic activity. Variations of solar wind parameters and geomagnetic activity indices following the shock arrival are explored. An interval of 6 h (3 days) following the shock is characterized by the average peak values of solar wind speed Vsw=525(610) km s- 1, IMF Bz=-6.5(-11.1) nT, and electric field Ey=3.5(6.1) mV m- 1, followed by the average peak geomagnetic indices of Dst=-36(-83) nT, ap=56(92) nT, and AE=733(1061) nT. About 25% and 63% of the shocks are followed by geomagnetic storms with Dst ≤ - 50 nT in the following 6-h and 3-day periods, respectively. The percentages of shocks followed by the auroral activity level AE > 500 nT are ≈ 65 % and ≈ 96 % for the short and long intervals, respectively. For the ap activity level (> 56 nT), the geoeffective shocks are ≈ 30 % and ≈ 60 %, respectively. The overall increase in the geomagnetic activity after the shock arrival for the longer shock-preceded interval is possibly due to inclusion of contributions from shock driver (ICME or CIR) fields. It can be concluded that an interplanetary fast forward shock has a probability of 1/4 to be followed by geomagnetic storms, and of 2/3 to be followed by significant auroral activity. We derived probability distribution functions of geomagnetic indices for the 6-h and 3-day intervals following shocks. The results might be important for space weather modeling and applications.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Geomagnetic Activity Following...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 03/05/2023 09:49 1.0 KiB 
4. Condições de acesso e uso
Idiomaen
Arquivo Alvos13538-023-01294-w.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/46KTFK8
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
DivulgaçãoWEBSCI; PORTALCAPES; SCIELO; SCOPUS.
Acervo Hospedeirourlib.net/www/2021/06.04.03.40
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
e-Mail (login)simone
atualizar 

1. Identificação
Tipo de ReferênciaResumo em Evento (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3SR84R5
Repositóriosid.inpe.br/mtc-m21c/2019/02.28.16.53
Última Atualização2019:02.28.16.53.18 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2019/02.28.16.53.18
Última Atualização dos Metadados2021:02.06.22.00.22 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoTsurutaniGTASBGAE:1988:InMaPh
TítuloInterplanetary magnetic phenomena and processes and the resultant control of geomagnetic activity at earth
Ano1988
Data de Acesso19 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho21 KiB
2. Contextualização
Autor1 Tsurutani, Bruce T.
2 Gonzalez Alarcon, Walter Demétrio
3 Tang, Frances
4 Akasofu, Syun I.
5 Smith, Edward J.
6 Brinca, Armando L.
7 Goldstein, Bruce E.
8 Anderson, Roger R.
9 Eastman, Timothy E.
Grupo1
2 DGE-INPE-BR
Afiliação1 Jet Propulsion Laboratory, California Institute of Technology
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 California Institute of Technology
4 Geophysical Institute
5 Jet Propulsion Laboratory, California Institute of Technology
6 Jet Propulsion Laboratory, California Institute of Technology
7 Jet Propulsion Laboratory, California Institute of Technology
8 University of Iowa
9 NASA Headquarters
Endereço de e-Mail do Autor1
2 walter.alarcon@inpe.br
EditorCosta, José Marques da
Kantor, Ivan Jelinek
Nordemann, Daniel Jean R.
Nome do EventoLatin-American Conference on Space Geophysics, 1
Localização do EventoÁguas de Lindóia, SP
Data21-25 nov.
Editora (Publisher)INPE
Cidade da EditoraSão José dos Campos, SP
Páginas33
Título do LivroAbstracts
Histórico (UTC)2019-02-28 16:53:18 :: simone -> administrator ::
2021-02-06 22:00:22 :: administrator -> simone :: 1988
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo de Versãopublisher
ÁreaCEA
ArranjoInterplanetary magnetic phenomena...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 28/02/2019 13:53 1.0 KiB 
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34R/3SR84R5
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34R/3SR84R5
Idiomaen
Arquivo Alvotsurutani_interplanetary.pdf
Grupo de Usuáriossimone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhourlib.net/www/2017/11.22.19.04.03
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosabstract archivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition format isbn issn keywords label lineage mark nextedition notes numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url volume
7. Controle da descrição
e-Mail (login)simone
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemarte3.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YCT/H3QRi
Repositóriosid.inpe.br/iris@1905/2005/08.04.06.45
Última Atualização2021:02.27.18.22.23 (UTC) marciana
Repositório de Metadadossid.inpe.br/iris@1905/2005/08.04.06.45.49
Última Atualização dos Metadados2021:02.27.18.22.24 (UTC) marciana
Rótulo10791
Chave de CitaçãoEcherGonz:2002:InShGe
TítuloInterplanetary shocks and geomagnetic activity in solar maximum (2002)and solar minimum (1995-1996)
Ano2002
Data Secundária20021220
Data de Acesso19 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho66 KiB
2. Contextualização
Autor1 Echer, E.
2 Gonzalez, Walter Demétrio
Grupo1 DGE-INPE-MCT-BR
Nome do EventoCOSPAR Scientific Assembly, the World Space Congress,35.
Localização do EventoHouston, USA
Data2002
Histórico (UTC)2018-06-06 03:56:15 :: administrator -> marciana :: 2002
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveGEOFÍSICA ESPACIAL
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Interplanetary shocks and...
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/6qtX3pFwXQZ3r59YCT/H3QRi
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZ3r59YCT/H3QRi
Arquivo Alvoecher_interplanetary.pdf
Grupo de Usuáriosadministrator
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 1
Acervo Hospedeirosid.inpe.br/banon/2001/04.03.15.36
6. Notas
Campos Vaziosabstract affiliation archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn language lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
e-Mail (login)marciana
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3S29A9P
Repositóriosid.inpe.br/mtc-m21c/2018/10.10.12.08
Última Atualização2018:10.10.12.08.30 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21c/2018/10.10.12.08.30
Última Atualização dos Metadados2019:04.06.04.53.15 (UTC) administrator
DOI10.1029/2018JA025683
ISSN2169-9402
Chave de CitaçãoRawatEcheGonz:2018:HoDiAr
TítuloHow Different Are the Solar Wind-Interplanetary Conditions and the Consequent Geomagnetic Activity During the Ascending and Early Descending Phases of the Solar Cycles 23 and 24?
Ano2018
MêsAug.
Data de Acesso19 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2618 KiB
2. Contextualização
Autor1 Rawat, Rashmi
2 Echer, Ezequiel
3 Gonzalez Alarcon, Walter Demétrio
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JH3D
3 8JMKD3MGP5W/3C9JJC4
ORCID1 0000-0002-5917-8693
2 0000-0002-8351-6779
3 0000-0002-4859-9310
Grupo1
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 National Centre for Antarctic and Ocean Research
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2 ezequiel.echer@inpe.br
3 walter.gonzalez@inpe.br
RevistaJournal of Geophysical Research: Space Physics
Volume123
Número8
Páginas6621-6638
Histórico (UTC)2018-10-10 12:08:30 :: simone -> administrator ::
2018-10-10 12:08:30 :: administrator -> simone :: 2018
2018-10-10 12:08:47 :: simone -> administrator :: 2018
2019-04-06 04:53:15 :: 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
ResumoThe current work investigates the possible solar wind-interplanetary (SW-IP) drivers of geomagnetic storms during the longest period (ascending to early descending phases) of the ongoing solar cycle (24). We present a comparative analysis between the two consecutive solar cycles (SCs) 23 and 24. Both the cycles exhibited dual peak feature as observed in the smoothed sunspot numbers SSNsmoothed. For both the cycles, second peak in the SSNsmoothed is higher than the first one as exhibited in the revised SSNsmoothed version. During the entire interval between the ascending to early descending phases (December 2008 to December 2016) of SC-24, the southward directed Bz and the dawn-dusk electric field (Ey) were consistently weaker as compared to that during similar interval of SC-23 (May 1996 to July 2004). The geomagnetic field response represented by Dst index concurrently exhibited similar variation patterns during both the periods. A striking reduction in the intense storm occurrence rate by ∼75% was observed during the considered period of the current solar cycle in comparison to the previous cycle. However, moderate storm occurrence was reduced only by 32% in SC-24 as compared to SC-23, which could be attributed to the dominance of corotating interaction regions during SC-24. No significant difference is found between the intense storm rates around the vernal and autumnal equinoxes in cycle 24, whereas distinct autumnal equinoctial dominance is evident for cycle 23. Further, within each cycle, there is no significant difference in the moderate storm rates around vernal and autumnal equinoxes.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > How Different Are...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 10/10/2018 09:08 1.0 KiB 
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34R/3S29A9P
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34R/3S29A9P
Idiomaen
Arquivo Alvorawat_how.pdf
Grupo de Usuáriossimone
Visibilidadeshown
Política de Arquivamentodenypublisher6 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 2
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 1
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
e-Mail (login)simone
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemarte3.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YCT/GUK4T
Repositóriosid.inpe.br/iris@1905/2005/07.29.22.07
Última Atualização2017:12.05.14.08.55 (UTC) marciana
Repositório de Metadadossid.inpe.br/iris@1905/2005/07.29.22.07.20
Última Atualização dos Metadados2018:06.06.04.03.48 (UTC) administrator
Chave SecundáriaINPE-7441-PRE/3330
ISSN0094-8276
Rótulo8735
Chave de CitaçãoGonzalez-AlerconTsurMcinGonz:1996:CoHoRe
TítuloCoranal hole-active region-current sheet (CHARCS) asociation with intense interplanetary and geomagnetic activity
ProjetoPROJETO MAGHEL
Ano1996
Data Secundária20000126
MêsSept.
Data de Acesso19 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho189 KiB
2. Contextualização
Autor1 Gonzalez-Alercon, Walter Demetrio
2 Tsurutani, B. T.
3 Mcintosh, P.
4 Gonzalez-Alarcon, Alicia Luisa Clua
Grupo1 DGE-INPE-MCT-BR
RevistaGeophysical Research Letters
Volume23
Número19
Páginas2577-2580
Histórico (UTC)2014-09-29 15:13:41 :: administrator -> marciana :: 1996
2017-12-05 14:08:56 :: marciana -> administrator :: 1996
2018-06-06 04:03:48 :: administrator -> marciana :: 1996
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveGEOFISICA ESPACIAL
TEMPESTADES MAGNETICAS
MAGNETOSFERA
ResumoIntense geomagnetic storms (Dst ... -100 nT) have been associated with interplanetary structureres involving large-intensity (B... 10 nT) and long duration (T ...3 hours) values of the southward component of the IMF. We show that near solar maximum, the solar origin of such structures seems to be associated with active regions* (involving flares and/ or filament eruptions) occurring close to the streamer belt and to growing low-latitude coronal holes. It is also shown that low-latitude coronal holes had a dual-peak solar cycle distribution during solar cycle 21, similar to that previously reported for the above mentioned interplanetary and geomagnetic phenomena.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Coranal hole-active region-current...
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/6qtX3pFwXQZ3r59YCT/GUK4T
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZ3r59YCT/GUK4T
Arquivo Alvo7441.pdf
Grupo de Usuáriosadministrator
Grupo de Leitoresadministrator
marciana
Visibilidadeshown
Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
DivulgaçãoWEBSCI; PORTALCAPES; SCIELO; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2001/04.03.15.36
6. Notas
Campos Vaziosaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readpermission resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
e-Mail (login)marciana
atualizar