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A expressão de busca foi <secondaryty pi and firstg DGE-CEA-INPE-MCTI-GOV-BR and y 2014 and dissemination websci>.
31 referências foram encontradas buscando em 15 dentre 15 sites
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As 10 mais recentes estão listadas abaixo.
Data e hora local de busca: 19/10/2020 13:22.

Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP7W/3G2HKDL
Repositóriosid.inpe.br/mtc-m19/2014/03.26.15.39
Metadadossid.inpe.br/mtc-m19/2014/03.26.15.39.19
Sitemtc-m16d.sid.inpe.br
DOI10.1002/2014GL059383
Rótuloself-archiving-INPE-MCTI-GOV-BR
ISSN0094-8276
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoHajraTsurEcheGonz:2014:SoCyPh
Autor1 Hajra, Rajkumar
2 Tsurutani, Bruce T.
3 Echer, Ezequiel
4 Gonzalez, Walter Demetrio
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JH3D
4 8JMKD3MGP5W/3C9JJC4
Grupo1
2
3 DGE-CEA-INPE-MCTI-GOV-BR
4 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Jet Propulsion Laboratory (JPL) - California Institute of Technology
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 rajkumarhajra@yahoo.co.in
2
3 eecher@dge.inpe.br
4 gonzalez@dge.inpe.br
TítuloRelativistic electron acceleration during high-intensity, long-duration, continuous AE activity (HILDCAA) events: solar cycle phase dependences
RevistaGeophysical Research Letters
Ano2014
Volume41
Número6
MêsMar.
Palavras-ChaveHILDCAAs, magnetospheric relativistic electrons, chorus waves, high-speed streams, Alfvén waves, solar cycle phases.
ResumoHigh-intensity, long-duration, continuous AE activity (HILDCAA) intervals during solar cycle 23 (19952008) have been studied by a superposed epoch analysis. It was found that HILDCAA intervals order the solar wind velocity, temperature and density (characteristic of high-speed solar wind intervals), the polar cap potential, and various other geomagnetic indices well. The interplanetary magnetic field Bz is generally negative, and the Newell solar wind coupling function is high during HILDCAA events. The HILDCAA intervals are well correlated with an enhancement of magnetospheric relativistic (E > 2 MeV) electron fluxes observed at geosynchronous orbit with a delay of ~1.5 days from the onset of the HILDCAAs. The response of the energetic electrons to HILDCAAs is found to vary with solar cycle phase. The initial electron fluxes are lower for events occurring during the ascending and solar maximum (AMAX) phases than for events occurring during the descending and solar minimum (DMIN) phases. The flux increases for the DMIN phase events are >50% larger than for the AMAX phase events. Although the solar wind speeds during the DMIN phases were slightly higher and lasted longer than during the AMAX phases, no other significant solar wind differences were noted. It is concluded that electrons are accelerated to relativistic energies most often and most efficiently during the DMIN phases of the solar cycle. We propose two possible solar UV mechanisms to explain this solar cycle effect.
Páginas1876–1881
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; AGU; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaA1_ENGENHARIAS_I A1_INTERDISCIPLINAR A1_CIÊNCIAS_AMBIENTAIS A1_GEOCIÊNCIAS A1_BIODIVERSIDADE A1_ENGENHARIAS_III A1_CIÊNCIAS_AGRÁRIAS_I A1_GEOGRAFIA A2_QUÍMICA A2_CIÊNCIAS_BIOLÓGICAS_I A2_ENGENHARIAS_II A2_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_ENSINO
Tamanho185 KiB
Número de Arquivos1
Arquivo AlvoRevisedManuscript.pdf
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Tipo do ConteudoExternal Contribution
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Tipo de Versãofinaldraft
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Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP7W/3G2HK4P
Repositóriosid.inpe.br/mtc-m19/2014/03.26.15.35
Metadadossid.inpe.br/mtc-m19/2014/03.26.15.35.23
Sitemtc-m16d.sid.inpe.br
DOI10.1002/2013JA019646
Rótuloself-archiving-INPE-MCTI-GOV-BR
ISSN2169-9402
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoHajraEcheTsurGonz:2014:HIPrCI
Autor1 Hajra, Rajkumar
2 Echer, Ezequiel
3 Tsurutani, Bruce T.
4 Gonzalez, Walter Demetrio
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JH3D
3
4 8JMKD3MGP5W/3C9JJC4
Grupo1
2 DGE-CEA-INPE-MCTI-GOV-BR
3
4 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Jet Propulsion Laboratory (JPL) - California Institute of Technology
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 rajkumarhajra@yahoo.co.in
2 eecher@dge.inpe.br
3
4 gonzalez@dge.inpe.br
TítuloSolar wind-magnetosphere energy coupling efficiency and partitioning: HILDCAAs and preceding CIR storms during solar cycle 23
RevistaJournal of Geophysical Research: Space Physics
Ano2014
Volume119
Número4
MêsApr.
Palavras-Chavesolar wind-magnetosphere energy coupling efficiency, magnetospheric energy partitioning, HILDCAAs, CIR storms, joule heating, ring current injection.
ResumoA quantitative study on the energetics of the solar wind-magnetosphere-ionosphere system during High-Intensity, Long-Duration, Continuous AE Activity (HILDCAA) events for solar cycle 23 (from 1995 through 2008) is presented. For all HILDCAAs, the average energy transferred to the magnetospheric/ionospheric system was ~6.3 ×1016 J, and the ram kinetic energy of the incident solar wind was ~7.1 ×1018 J. For individual HILDCAA events the coupling efficiency, defined as the ratio of the solar wind energy input to the solar wind kinetic energy, varied between 0.3% and 2.8%, with an average value of ~0.9%. The solar wind coupling efficiency for corotating interaction region (CIR)-driven storms prior to the HILDCAA events was found to vary from ~1% to 5%, with an average value of ~2%. Both of these values are lower than the> 5% coupling efficiency noted for interplanetary coronal mass ejection (and sheath)-driven magnetic storms. During HILDCAAs, ~67% of the solar wind energy input went into Joule heating, ~22% into auroral precipitation, and ~11% into the ring current energy. The CIR-storm Joule heating (~49%) was noticeably less than that during HILDCAAs, while the ring current energies were comparable for the two. Joule dissipation was higher for HILDCAAs that followed CIR-storms (88%) than for isolated HILDCAAs (~60%). Possible physical interpretations for the statistical results obtained in this paper are discussed.
Páginas2675–2690
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; AGU; COMPENDEX; SCOPUS.
AreaCEA
ProjetoCNPq (301233/2011-0)
Tamanho327 KiB
Número de Arquivos1
Arquivo AlvoRevisedManuscript.pdf
Última Atualização2014:03.26.15.35.23 sid.inpe.br/mtc-m19@80/2009/08.21.17.02 administrator
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Tipo do ConteudoExternal Contribution
Estágio do Documentonot transferred
Tipo de Versãofinaldraft
Política de Arquivamentodenypublisher6 allowfinaldraft
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 26/03/2014 12:35 1.0 KiB 
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Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP7W/3E9B8AD
Repositóriosid.inpe.br/mtc-m19/2013/06.09.02.20.08   (acesso restrito)
Metadadossid.inpe.br/mtc-m19/2013/06.09.02.20.09
Sitemtc-m16d.sid.inpe.br
DOI10.1016/j.atmosres.2013.01.008
Rótuloscopus
ISSN0169-8095
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoZepkaPintSara:2014:LiFoSo
Autor1 Zepka, Gisele dos Santos
2 Pinto Junior, Osmar
3 Saraiva, Antonio Carlos Varela
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JJ2E
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 CST-CST-SPG-INPE-MCTI-GOV-BR
3 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 giselezepka@gmail.com
2 osmar@dge.inpe.br
3 antonio@dge.inpe.br
TítuloLightning forecasting in southeastern Brazil using the WRF model
RevistaAtmospheric Research
Ano2014
Volume135-136
MêsJan.
Palavras-Chavelightning, WRF model, forecasting, parameterization, convection, microphysics.
ResumoThis paper introduces a lightning forecasting method called Potential Lightning Region (PLR), which is the probability of the occurrence of lightning over a region of interest. The PLR was calculated using a combination of meteorological variables obtained from high-resolution Weather Research and Forecasting (WRF) model simulations during the summer season in southeastern Brazil. The model parameters used in the PLR definition were: surface-based Convective Available Potential Energy (SBCAPE), Lifted Index (LI), K-Index (KI), average vertical velocity between 850 and 700 hPa (w), and integrated ice-mixing ratio from 700 to 500 hPa (QICE). Short-range runs of twelve non-severe thunderstorm cases were performed with the WRF model, using different convective and microphysical schemes. Through statistical evaluations, the WRF cloud parameterizations that best described the convective thunderstorms with lightning in southeastern Brazil were the combination of Grell-Devenyi and Thompson schemes. Two calculation methods were proposed: the Linear PLR and Normalized PLR. The difference between them is basically how they deal with the influence of lightning flashes over the WRF domain's grid points for the twelve thunderstorms analyzed. Three case studies were used to test both methods. A statistical evaluation lowering the spatial resolution of the WRF grid into larger areas was performed to study the behavior and accuracy of the PLR methods. The Normalized PLR presented the most suitable one, predicting flash occurrence appropriately. © 2013 Elsevier B.V. All rights reserved.
Páginas344–362
Idioma{{mtc-m16d.sid.inpe.br 806} sid.inpe.br/mtc-m19@80/2009/08.21.17.02 USP}
URL (dados não confiáveis)http://dx.doi.org/10.1016/j.atmosres.2013.01.008
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaA1_CIÊNCIAS_AMBIENTAIS A1_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_CIÊNCIAS_AGRÁRIAS_I B1_ENGENHARIAS_IV B1_BIODIVERSIDADE B1_ENGENHARIAS_II B1_MATEMÁTICA_/_PROBABILIDADE_E B1_ENGENHARIAS_III B2_ASTRONOMIA_/_FÍSICA
Tamanho6486 KiB
Número de Arquivos1
Arquivo Alvo1-s2.0-S0169809513000458-main.pdf
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Estágio do Documentonot transferred
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Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W/3HEJGFB
Repositóriosid.inpe.br/plutao/2014/11.21.17.48   (acesso restrito)
Metadadossid.inpe.br/plutao/2014/11.21.17.48.31
Siteplutao.sid.inpe.br
DOI10.1186/s40623-014-0151-5
Rótuloself-archiving-INPE-MCTI-GOV-BR
ISSN1343-8832
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoKozaiMKKBERLSTDHSJSK:2014:SpDeGr
Autor 1 Kozai, Masayoshi
 2 Munakata, Kazuoki
 3 Kato, Chihiro
 4 Kuwabara, Takao
 5 Bieber, John W
 6 Evenson, Paul
 7 Rockenbach, Marlos
 8 Lago, Alisson Dal
 9 Schuch, Nelson Jorge
10 Tokumaru, Munetoshi
11 Duldig, Marcus L
12 Humble, John E
13 Sabbah, Ismail
14 Jassar, Hala K Al
15 Sharma, Madan M
16 Kóta, Jozsef
Identificador de Curriculo 1
 2
 3
 4
 5
 6
 7
 8 8JMKD3MGP5W/3C9JGH3
 9 8JMKD3MGP5W/3C9JHUD
Grupo 1
 2
 3
 4
 5
 6
 7
 8 DGE-CEA-INPE-MCTI-GOV-BR
 9 CRS-CCR-INPE-MCTI-GOV-BR
Afiliação 1
 2
 3
 4
 5
 6
 7
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor 1
 2
 3
 4
 5
 6
 7
 8 alisson.dallago@inpe.br
 9 njschuch@lacesm.ufsm.br
TítuloThe spatial density gradient of galactic cosmic rays and its solar cycle variation observed with the Global Muon Detector Network
RevistaEarth, Planets and Space
Ano2014
Volume66
Número151
Palavras-ChaveDiurnal anisotropy, North-south anisotropy, Heliospheric modulation of galactic cosmic rays, Solar cycle variation of the cosmic ray density gradient.
ResumoWe derive the long-term variation of the three-dimensional (3D) anisotropy of approximately 60 GV galactic cosmic rays (GCRs) from the data observed with the Global Muon Detector Network (GMDN) on an hourly basis and compare it with the variation deduced from a conventional analysis of the data recorded by a single muon detector at Nagoya in Japan. The conventional analysis uses a north-south (NS) component responsive to slightly higher rigidity (approximately 80 GV) GCRs and an ecliptic component responsive to the same rigidity as the GMDN. In contrast, the GMDN provides all components at the same rigidity simultaneously. It is confirmed that the temporal variations of the 3D anisotropy vectors including the NS component derived from two analyses are fairly consistent with each other as far as the yearly mean value is concerned. We particularly compare the NS anisotropies deduced from two analyses statistically by analyzing the distributions of the NS anisotropy on hourly and daily bases. It is found that the hourly mean NS anisotropy observed by Nagoya shows a larger spread than the daily mean due to the local time-dependent contribution from the ecliptic anisotropy. The NS anisotropy derived from the GMDN, on the other hand, shows similar distribution on both the daily and hourly bases, indicating that the NS anisotropy is successfully observed by the GMDN, free from the contribution of the ecliptic anisotropy. By analyzing the NS anisotropy deduced from neutron monitor (NM) data responding to lower rigidity (approximately 17 GV) GCRs, we qualitatively confirm the rigidity dependence of the NS anisotropy in which the GMDN has an intermediate rigidity response between NMs and Nagoya. From the 3D anisotropy vector (corrected for the solar wind convection and the Compton-Getting effect arising from the Earths orbital motion around the Sun), we deduce the variation of each modulation parameter, i.e., the radial and latitudinal density gradients and the parallel mean free path for the pitch angle scattering of GCRs in the turbulent interplanetary magnetic field. We show the derived density gradient and mean free path varying with the solar activity and magnetic cycles.
Páginas1-8
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
AreaCEA
Nota SecundáriaB1_GEOCIÊNCIAS B1_ENGENHARIAS_I B1_ANTROPOLOGIA_/_ARQUEOLOGIA B4_ASTRONOMIA_/_FÍSICA B4_SOCIOLOGIA
Nota TerciáriaTrabalho não Vinculado à Tese/Dissertação
Tamanho693 KiB
Número de Arquivos1
Arquivo AlvoKozai_Spatial.pdf
Última Atualização2015:02.11.11.25.01 dpi.inpe.br/plutao@80/2008/08.19.15.01 administrator
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8JMKD3MGPCW/3EUFCFP
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Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarytype url
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W/3GDQQT5
Repositóriosid.inpe.br/plutao/2014/06.03.22.53   (acesso restrito)
Metadadossid.inpe.br/plutao/2014/06.03.22.53.24
Siteplutao.sid.inpe.br
DOI10.1051/swsc/2013056
Rótulolattes: 3368023405805386 6 TsurutaniESVMGKP:2014:CAIIOv
ISSN2115-7251
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoTsurutaniESVMGKP:2014:CAIIOv
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
TítuloThe interplanetary causes of geomagnetic activity during the 7-17 March 2012 interval: a CAWSES II overview
RevistaJournal of Space Weather and Space Climate
Ano2014
Volume4
Palavras-ChaveAtividade Geomagnetica, Geomagnetic storms.
PáginasA02
NotasSetores de Atividade: Pesquisa e desenvolvimento científico.
Idiomaen
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
AreaCEA
Nota SecundáriaB5_GEOCIÊNCIAS
Tamanho1315 KiB
Número de Arquivos1
Arquivo AlvoTsurutani_2014swscCAWSESII.pdf
Última Atualização2014:07.17.16.39.45 dpi.inpe.br/plutao@80/2008/08.19.15.01 administrator
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Permissão de Leituradeny from all and allow from 150.163
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2018-06-04 23:39:32 :: administrator -> marcelo.pazos@inpe.br :: 2014
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 secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W/3GDQM5S
Repositóriosid.inpe.br/plutao/2014/06.03.22.07
Metadadossid.inpe.br/plutao/2014/06.03.22.07.28
Siteplutao.sid.inpe.br
DOI10.5194/acpd-14-12279-2014
Rótulolattes: 9873289111461387 8 BritoRMCJHLFAA:2014:GrBaAe
ISSN1680-7367
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoBritoRMCJHFFAA:2014:GrBaAe
Autor 1 Brito, J.
 2 Rizzo, L. V.
 3 Morgan, W. T.
 4 Coe, H.
 5 Johnson, B.
 6 Haywood, J.
 7 Freitas, Karla Maria Longo de
 8 Freitas, Saulo Ribeiro de
 9 Andreae, M. O.
10 Artaxo, P.
Identificador de Curriculo 1
 2
 3
 4
 5
 6
 7
 8 8JMKD3MGP5W/3C9JJ7M
Grupo 1
 2
 3
 4
 5
 6
 7 DGE-CEA-INPE-MCTI-GOV-BR
 8 DMD-CPT-INPE-MCTI-GOV-BR
Afiliação 1 University of São Paulo
 2 Federal University of São Paulo
 3 University of Manchester
 4 University of Manchester
 5 UK Met Office
 6 UK Met Office
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Max Planck Institute for Chemistry
10 University of São Paulo
Endereço de e-Mail do Autor 1
 2
 3
 4
 5
 6
 7 karla.longo@inpe.br
 8 sfreitas@cptec.inpe.br
TítuloGround based aerosol characterization during the South American Biomass Burning Analysis (SAMBBA) field experiment
RevistaAtmospheric Chemistry and Physics Discussions
Ano2014
Volume14
Número8
Palavras-Chaveaerosol, South American Biomass Burning Analysis.
ResumoThis paper investigates the physical and chemical characteristics of aerosols at ground level at a site heavily impacted by biomass burning. The site is located near Porto Velho, Rondônia, in the Southwestern part of the Brazilian Amazon forest, and was selected for the deployment of a large suite of instruments, among them an Aerosol Chemical Speciation Monitor. Our measurements were made during the South American Biomass Burning Analysis (SAMBBA) field experiment, which consisted of a combination of aircraft and ground based measurements over Brazil, aiming to investigate the impacts of biomass burning emissions on climate, air quality, and numerical weather prediction over South America. The campaign took place during the dry season and the transition to the wet season in September/October 2012. During most of the campaign, the site was impacted by regional biomass burning pollution (average CO mixing ratio of 0.6 ppm), occasionally superimposed by intense (up to 2 ppm of CO), freshly emitted biomass burning plumes. Aerosol number concentrations ranged from ∼1000 cm−3 to peaks of up to 35 000 cm−3 during biomass burning (BB) events, corresponding to an average submicron mass mean concentrations of 13.7 μg m−3 and peak concentrations close to 100 μg m−3. Organic aerosol strongly dominated the submicron non-refractory composition, with an average concentration of 11.4 μg m−3. The inorganic species, NH4, SO4, NO3, and Cl, were observed on average at concentrations of 0.44, 0.34, 0.19, and 0.01 μg m−3, respectively. Equivalent Black Carbon (BCe) ranged from 0.2 to 5.5 μg m−3, with an average concentration of 1.3 μg m−3. During BB peaks, organics accounted for over 90% of total mass (submicron non-refractory plus BCe), among the highest values described in the literature. We examined the ageing of Biomass Burning Organic Aerosol (BBOA) using the changes in the H : C and O : C ratios, and found that throughout most of the aerosol processing (O : C ≅ 0.25 to O : C ≅ 0.6), no remarkable change is observed in the H : C ratio (∼1.35). Such a result contrasts strongly with previous observations of chemical ageing of both urban and Amazonian biogenic aerosols. At higher levels of processing (O : C>0.6), the H : C ratio changes with a H : C / O : C slope of −0.5, possibly due to the development of a combination of BB (H : C / O : C slope = 0) and biogenic (H : C / O : C slope = −1) OA. An analysis of the ΔOA / ΔCO mass ratios yields very little enhancement in the OA loading with atmospheric processing, consistent with previous observations. These results indicate that negligible Secondary Organic Aerosol (SOA) formation occurs throughout the observed BB plume processing, or that SOA formation is almost entirely balanced by OA volatilization. Positive Matrix Factorization of the organic aerosol spectra resulted in three factors: Fresh BBOA, Aged BBOA and Low-Volatility Oxygenated Organic Aerosol (LV-OOA). Analysis of the diurnal patterns and correlation with external markers indicates that during the first part of the campaign OA concentrations are impacted by local fire plumes with some chemical processing occurring in the near-surface layer. During the second part of the campaign, long-range transport of BB plumes above the surface layer, as well as potential SOAs formed aloft, dominates OA concentrations at our ground-based sampling site. This manuscript describes the first ground-based deployment of aerosol mass spectrometry at a site heavily impacted by biomass burning in the Amazon region, allowing a deeper understanding of aerosol life cycle in this important ecosystem.
Páginas12279-12322
Idiomaen
URL (dados não confiáveis)http://www.atmos-chem-phys-discuss.net/acpd-14-12279-2014/
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
AreaCEA
Nota SecundáriaC_ASTRONOMIA_/_FÍSICA
Tamanho11711 KiB
Número de Arquivos3
Arquivo Alvoacp-14-12069-2014-supplement.pdf
Última Atualização2014:12.09.12.50.51 dpi.inpe.br/plutao@80/2008/08.19.15.01 administrator
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Estágio do Documentonot transferred
Repositório de Direitos Autoraisurlib.net/www/2012/11.12.14.05
Tipo de Versãopublisher
Política de Arquivamentoallowpublisher allowfinaldraft
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
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Histórico2014-06-03 22:07:28 :: lattes -> administrator ::
2018-06-04 23:39:31 :: administrator -> marcelo.pazos@inpe.br :: 2014
Campos Vaziosalternatejournal archivist callnumber copyholder creatorhistory descriptionlevel format isbn lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3HP89BB
Repositóriosid.inpe.br/mtc-m21b/2015/01.13.18.16.48   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2015/01.13.18.16.49
Sitemtc-m21b.sid.inpe.br
DOI10.1016/j.palaeo.2014.07.019
Rótuloscopus 2015-01 EvangelistaGurSifRigBou:2014:SoTrAt
ISSN0031-0182
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoEvangelistaGurSifRigBou:2014:SoTrAt
Autor1 Evangelista, Heitor
2 Gurgel, Marcio
3 Sifeddine, Abdelfettah
4 Rigozo, Nivaor Rodolfo
5 Boussafir, Mohammed
Grupo1
2
3
4 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 LARAMG - Lab. de Radioecologia e Mudanças Globais/DBB/IBRAG/Uni. do Estado do Rio de Janeiro, Pavilhão Haroldo L. Cunha, Subsolo, Rua São Francisco Xavier, 524, MaracanãRio de Janeiro, RJ, Brazil
2 School of Arts, Sciences and Humanities, University of São PauloSão Paulo, Brazil; Av. Arlindo Bettio, 1000São Paulo, SP, Brazil
3 Departamento de Geoquimica, Universidade Federal Fluminense, Departamento de Geoquímica/IQ, Morro de Valongunho S/n, 5 AndarCentro, Niterói, RJ, Brazil; IRD-LOCEAN (UMR 7159 IRD/CNRS/UPMC/MNHN)-Institut Pierre-Simon LaplaceBondy, France
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 IRD-LOCEAN (UMR 7159 IRD/CNRS/UPMC/MNHN)-Institut Pierre-Simon LaplaceBondy, France
TítuloSouth Tropical Atlantic anti-phase response to Holocene Bond Events
RevistaPalaeogeography, Palaeoclimatology, Palaeoecology
Ano2014
Volume415
Palavras-Chavealkenone, climate change, climate effect, hematite, Holocene, sea surface temperature, sediment core, time series, Atlantic Ocean, Atlantic Ocean (Tropical), Brazil, Caribbean Sea, Gulf of Caraico, Rio de Janeiro [Brazil].
ResumoRecords of the climatic impacts of the North Atlantic Bond cycles over the subtropical Southern Hemisphere remain scarce, and their mechanism is a topic of active discussion. We present here an alkenone-based reconstructed sea surface temperature (SST) of a sediment core retrieved from the Brazilian Southwestern Tropical Atlantic (SWTA), Rio de Janeiro, together with a sediment SST record from the Cariaco Basin. The sediment cores span the period 2,100 B.P. - 11,100 B.P. Morlet-wavelet analysis detected marked periodic signals of ~. 0.8, ~. 1.7 and ~. 2.2. kyr, very similar and with comparable phases to the hematite-stained-grain time series from the Northern North Atlantic in which the cyclic pattern was recognized as Bond cycles. Our result corroborates the modeled surface ocean anti-phase thermal relation between the North and the South Atlantic. We attribute this behavior to the slowing of the Atlantic Meridional Overturning Circulation. The relative SST warming at Rio de Janeiro and the relative cooling at Cariaco were comparatively more pronounced during the early Holocene (from 11 to 5 kyr B.P.) than in more recent time.
Páginas21-27
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; AGU; SCOPUS.
AreaCEA
Nota SecundáriaA1_ENGENHARIAS_III A1_BIODIVERSIDADE A1_CIÊNCIAS_AMBIENTAIS A1_GEOGRAFIA A1_INTERDISCIPLINAR A2_CIÊNCIAS_AGRÁRIAS_I A2_GEOCIÊNCIAS A2_SAÚDE_COLETIVA B1_QUÍMICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_IV B2_ASTRONOMIA_/_FÍSICA C_FILOSOFIA/TEOLOGIA:subcomissão_FILOSOFIA
Nota TerciáriaTrabalho não Vinculado à Tese/Dissertação
Tamanho1592 KiB
Número de Arquivos1
Arquivo Alvo1-s2.0-S0031018214003745-main.pdf
Última Atualização2015:01.21.15.43.34 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator
Última Atualização dos Metadados2018:06.04.03.04.44 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2014}
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Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
Tipo do ConteudoExternal Contribution
Estágio do Documentonot transferred
Tipo de Versãopublisher
Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
Histórico2018-06-04 03:04:44 :: administrator -> marcelo.pazos@inpe.br :: 2014
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn lineage mark mirrorrepository month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarytype url
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP5W34M/3HE6STN
Repositóriosid.inpe.br/mtc-m21b/2014/11.19.02.18.29
Metadadossid.inpe.br/mtc-m21b/2014/11.19.02.18.30
Sitemtc-m21b.sid.inpe.br
DOI10.1088/0004-637X/793/1/6
Rótuloisi 2014-11 RemyaTsReLaFaEcGl:2014:LOPLBe
ISSN0004-637X
1538-4357
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoRemyaTsReLaFaEcGl:2014:LoPlBe
Autor1 Remya, B.
2 Tsurutani, B. T.
3 Reddy, R. V.
4 Lakhina, G. S.
5 Falkowski, B. J.
6 Echer, Ezequiel
7 Glassmeier, K. -H.
Identificador de Curriculo1
2
3
4
5
6 8JMKD3MGP5W/3C9JH3D
Grupo1
2
3
4
5
6 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Indian Inst Geomagnetism, Navi Mumbai, Maharashtra, India.
2 CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA.
3 Indian Inst Geomagnetism, Navi Mumbai, Maharashtra, India.
4 Indian Inst Geomagnetism, Navi Mumbai, Maharashtra, India.
5 CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA.
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 IGEP, D-38106 Braunschweig, Germany.
TítuloLarge-amplitude, circularly polarized, compressive, obliquely propagating electromagnetic proton cyclotron waves throughout the earth's magnetosheath: low plasma beta conditions
RevistaAstrophysical Journal
Ano2014
Volume793
Número1
MêsSep.
Palavras-Chaveinstabilities, methods: data analysis, planets and satellites: individual (Earth, Cassini, WIND), planets and satellites: magnetic fields, polarization.
ResumoDuring 1999 August 18, both Cassini and WIND were in the Earth's magnetosheath and detected transverse electromagnetic waves instead of the more typical mirror-mode emissions. The Cassini wave amplitudes were as large as similar to 14 nT (peak to peak) in a similar to 55 nT ambient magnetic field B-0. A new method of analysis is applied to study these waves. The general wave characteristics found were as follows. They were left-hand polarized and had frequencies in the spacecraft frame (f(scf)) below the proton cyclotron frequency (f(p)). Waves that were either right-hand polarized or had f(scf) > f(p) are shown to be consistent with Doppler-shifted left-hand waves with frequencies in the plasma frame f(pf) < f(p). Thus, almost all waves studied are consistent with their being electromagnetic proton cyclotron waves. Most of the waves (similar to 55%) were found to be propagating along B0 (theta(kB0) < 30 degrees), as expected from theory. However, a significant fraction of the waves were found to be propagating oblique to B0. These waves were also circularly polarized. This feature and the compressive ([B-max - B-min]/B-max, where B-max and B-min are the maximum and minimum field magnitudes) nature (ranging from 0.27 to 1.0) of the waves are noted but not well understood at this time. The proton cyclotron waves were shown to be quasi-coherent, theoretically allowing for rapid pitch-angle transport of resonant protons. Because Cassini traversed the entire subsolar magnetosheath and WIND was in the dusk-side flank of the magnetosheath, it is surmised that the entire region was filled with these waves. In agreement with past theory, it was the exceptionally low plasma beta (0.35) that led to the dominance of the proton cyclotron wave generation during this interval. A high-speed solar wind stream (< V-sw > = 598 km s(-1)) was the source of this low-beta plasma.
Idiomaen
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
AreaCEA
Nota TerciáriaTrabalho não Vinculado à Tese/Dissertação
Tamanho1609 KiB
Número de Arquivos1
Arquivo Alvo0004-637X_793_1_6remya.pdf
Última Atualização2015:01.16.13.26.00 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator
Última Atualização dos Metadados2018:06.04.03.04.35 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2014}
Estágio do Documentoconcluido
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Espelhoiconet.com.br/banon/2006/11.26.21.31
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marciana
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Estágio do Documentonot transferred
Tipo de Versãopublisher
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
Histórico2018-06-04 03:04:35 :: administrator -> marciana :: 2014
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn lineage mark nextedition notes orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarytype typeofwork url
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP5W34M/3HE6FMG
Repositóriosid.inpe.br/mtc-m21b/2014/11.19.00.02.02
Metadadossid.inpe.br/mtc-m21b/2014/11.19.00.02.03
Sitemtc-m21b.sid.inpe.br
DOI10.5194/npg-21-1059-2014
Rótuloscopus 2014-11 OjedaGonzálezGonMenDomRos:2014:NoFlAn
ISSN1023-5809
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoGonzálezGonMenDomRos:2014:NoFlAn
Autor1 González, Arian Ojeda
2 Gonzalez, Walter Demétrio
3 Mendes, Odim
4 Domingues, Margarete Oliveira
5 Rosa, Reinaldo Roberto
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JJC4
3
4 8JMKD3MGP5W/3C9JHQP
5 8JMKD3MGP5W/3C9JJ5D
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
3 DGE-CEA-INPE-MCTI-GOV-BR
4 LAC-CTE-INPE-MCTI-GOV-BR
5 LAC-CTE-INPE-MCTI-GOV-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)
TítuloNonlinear fluctuation analysis for a set of 41 magnetic clouds measured by the Advanced Composition Explorer (ACE) spacecraft
RevistaNonlinear Processes in Geophysics
Ano2014
Volume21
Número5
ResumoThe statistical distribution of values in the signal and the autocorrelations (interpreted as the memory or persistence) between values are attributes of a time series. The autocorrelation function values are positive in a time series with persistence, while they are negative in a time series with anti-persistence. The persistence of values with respect to each other can be strong, weak, or nonexistent. A strong correlation implies a " memory" of previous values in the time series. The long-range persistence in time series could be studied using semivariograms, rescaled range, detrended fluctuation analysis and Fourier spectral analysis, respectively. In this work, persistence analysis is to study interplanetary magnetic field (IMF) time series.We use data from the IMF components with a time resolution of 16 s. Time intervals corresponding to distinct processes around 41 magnetic clouds (MCs) in the period between March 1998 and December 2003 were selected. In this exploratory study, the purpose of this selection is to deal with the cases presenting the three periods: plasma sheath, MC, and post-MC. We calculated one exponent of persistence (e.g., ±, ², Hu, Ha) over the previous three time intervals. The persistence exponent values increased inside cloud regions, and it was possible to select the following threshold values:(±(j )i = 1.392, hHa(j )i = 0.327, and hHu(j )i=0.875. These values are useful as another test to evaluate the quality of the identification. If the cloud is well structured, then the persistence exponent values exceed thresholds. In 80.5% of the cases studied, these tools were able to separate the region of the cloud from neighboring regions. The Hausdorff exponent (Ha) provides the best results.
Páginas1059-1073
Idiomaen
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
AreaCEA
Nota SecundáriaA2_GEOCIÊNCIAS B1_MATEMÁTICA_/_PROBABILIDADE_E B1_BIODIVERSIDADE B1_ENGENHARIAS_IV B1_INTERDISCIPLINAR B2_CIÊNCIAS_BIOLÓGICAS_I B2_BIOTECNOLOGIA B3_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_AGRÁRIAS_I
Nota Terciária8JMKD3MGP7W/3DJMQKS
Tamanho1284 KiB
Número de Arquivos1
Última Atualização2014:12.30.16.28.39 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator
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Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
Tipo do ConteudoExternal Contribution
Estágio do Documentonot transferred
Tipo de Versãopublisher
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Unidades Imediatamente Superiores8JMKD3MGPCW/3ESGTTP
8JMKD3MGPCW/3EU29DP
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
Histórico2018-06-04 03:04:35 :: administrator -> marcelo.pazos@inpe.br :: 2014
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn keywords lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarytype typeofwork url
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP5W34M/3HE6FMA
Repositóriosid.inpe.br/mtc-m21b/2014/11.19.00.01.56
Metadadossid.inpe.br/mtc-m21b/2014/11.19.00.01.57
Sitemtc-m21b.sid.inpe.br
DOI10.1002/2014GL061157
Rótuloscopus 2014-11 WangLKVDNGSBLZFHW:2014:ObDoLa
ISSN0094-8276
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoWangLKVDNGSBLZFHW:2014:ObDoLa
Autor 1 Wang, R.
 2 Lu, Q.
 3 Khotyaintsev, Y. V.
 4 Volwerk, M.
 5 Du, A.
 6 Nakamura, R.
 7 Gonzalez, Walter Demétrio
 8 Sun, X.
 9 Baumjohann, W.
10 Li, X.
11 Zhang, T.
12 Fazakerley, A. N.
13 Huang, C.
14 Wu, M.
Identificador de Curriculo 1
 2
 3
 4
 5
 6
 7 8JMKD3MGP5W/3C9JJC4
Grupo 1
 2
 3
 4
 5
 6
 7 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação 1 Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
 2 Department of Geophysics and Planetary Science, University of Science and Technology of China, Hefei, China
 3 Swedish Institute of Space Physics, Uppsala, Sweden
 4 Space Research Institute, Austrian Academy of Sciences, Graz, Austria
 5 Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
 6 Space Research Institute, Austrian Academy of Sciences, Graz, Austria
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 School of Physics, University of Science and Technology of China, Hefei, China
 9 Space Research Institute, Austrian Academy of Sciences, Graz, Austria
10 Institute of Mathematics and Physics, Aberystwyth University, Aberystwyth, United Kingdom
11 Space Research Institute, Austrian Academy of Sciences, Graz, Austria
12 Mullard Space Science Laboratory, Surrey, United Kingdom
13 Department of Geophysics and Planetary Science, University of Science and Technology of China, Hefei, China
14 Department of Geophysics and Planetary Science, University of Science and Technology of China, Hefei, China
TítuloObservation of double layer in the separatrix region during magnetic reconnection
RevistaGeophysical Research Letters
Ano2014
Volume41
Número14
Palavras-ChaveEnergy dissipation, Beam distribution, Double layers, Electron hole, Electron measurements, In-situ observations, Magnetic reconnections, Parallel electric fields, Time resolution, Electrons, acoustic wave, electric field, electron, energy dissipation, magnetic field.
ResumoWe present in situ observation of double layer (DL) and associated electron measurement in the subspin time resolution in the separatrix region during reconnection for the first time. The DL is inferred to propagate away from the X line at a velocity of about ion acoustic speed and the parallel electric field carried by the DL can reach -20 mV/m. The electron displays a beam distribution inside the DL and streams toward the X line with a local electron Alfvén velocity. A series of electron holes moving toward the X line are observed in the wake of the DL. The identification of multiple similar DLs indicates that they are persistently produced and therefore might play an important role in energy conversion during reconnection. The observation suggests that energy dissipation during reconnection can occur in any region where the DL can reach. © 2014. American Geophysical Union. All Rights Reserved.
Páginas4851-4858
Idiomaen
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; AGU; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaA1_ENGENHARIAS_I A1_INTERDISCIPLINAR A1_CIÊNCIAS_AMBIENTAIS A1_GEOCIÊNCIAS A1_BIODIVERSIDADE A1_ENGENHARIAS_III A1_CIÊNCIAS_AGRÁRIAS_I A1_GEOGRAFIA A2_QUÍMICA A2_CIÊNCIAS_BIOLÓGICAS_I A2_ENGENHARIAS_II A2_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_ENSINO
Nota TerciáriaTrabalho não Vinculado à Tese/Dissertação
Tamanho1569 KiB
Número de Arquivos1
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Data de Acesso19 out. 2020
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