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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3JL4F75
Repositóriosid.inpe.br/mtc-m21b/2015/06.09.12.32
Metadadossid.inpe.br/mtc-m21b/2015/06.09.12.32.04
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Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoAdhikariMendDomiEche:2015:StFiAl
Autor1 Adhikari, Binod
2 Mendes Júnior, Odim
3 Domingues, Margarete Oliveira
4 Echer, Ezequiel
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JJ28
3 8JMKD3MGP5W/3C9JHQP
4 8JMKD3MGP5W/3C9JH3D
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
3 LAC-CTE-INPE-MCTI-GOV-BR
4 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)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 binod.adhi@gmail.com
2 odim.mendes@inpe.br
3 margarete.domingues@inpe.br
4 eecher@dge.inpe.br
TítuloStudy of field aligned current (FAC) with D-component (eastwest)and interplanetary electric field (Ey) during three different HILDCAA events
Nome do EventoJoin Assembly
Ano2015
Data3-7 may
Localização do EventoMontreal, Canada
ResumoField Aligned Currents (FACs) play an important role for the coupling between ionosphere and magnetosphere. This coupling is directly influenced by solar wind and interplanetary magnetic field (IMF). In this work we observe characteristics of FACs during HILDCAAs (High-Intensity, Long duration, Continuous AE activity) by using high resolution OMNI data set consisting of 1-min averaged ACE, Wind, IMP 8 and Geo-tail magnetic field. We also observe the perturbations in the ∆D (east-west) component of the geomagnetic field from the low latitude station (Vassouras) to predicate the field aligned currents. For three different HILDCAA events, the characteristics of FACs and perturbations in the ∆D component observe are quite dissimilar. The wavelet techniques (CWT, DWT and wavelet modulus correlation) and cross-correlation also show different results for each event. The times and frequencies resolution of FAC and ∆D obtained from CWT are different in each event. The nature of square wavelet coefficients obtain from DWT for FAC and ∆D are totally different. Both FAC and ∆D show good wavelet modulus correlation with components of interplanetary magnetic field (By and Bz) at the time of HILDCAA. We also observe the cross-correlation between FAC and ∆D, FAC and Ey and Ey and ∆D. During the non-storm HILDCAA, FAC shows negative correlation with ∆D. But it shows positive correlation for CIR and ICME preceding HILDCCAs. Similary, Ey and FAC also show negative correlation during non-storm HILDCAA but other two events show positive correlation. Finally, Ey and ∆D show positive correlation for all events. Observing these results, it can be suggested that the ground magnetic datasets obtained from low latitude may serve as the proxy for interplanetary conditions in the solar wind.
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3J33CRS
Repositóriosid.inpe.br/mtc-m21b/2015/02.24.17.01   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2015/02.24.17.01.15
Sitemtc-m21b.sid.inpe.br
DOI10.1007/s10714-014-1796-x
ISSN0001-7701
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoAstoneWABCDGKMNRSSVWABBCCCCCCCEGGHKLLMPPPPRSWWWWPP:2015:SeReDa
Autor 1 Astone, Pia
 2 Weinstein, Alan
 3 Agathos, Michalis
 4 Bejger, Michal
 5 Christensen, Nelson
 6 Dent, Thomas
 7 Graff, Philip
 8 Klimenko, Sergey
 9 Mazzolo, Giulio
10 Nishizawa, Atsushi
11 Robinet, Florent
12 Schmidit, Patricia
13 Smith, Rory
14 Veitch, John
15 Wade, Madeline
16 Aoudia, Sofiane
17 Bose, Sukanta
18 Bustillo, Juan Calderon
19 Canizares, Priscilla
20 Capano, Colin
21 Clark, James
22 Colla, Alberto
23 Cuoco, Elena
24 Costa, Carlos da Silva
25 Canton, Tito dal
26 Evangelista, Edgard de Freitas Diniz
27 Goetz, Evan
28 Gupta, Anuradha
29 Hannam, Mark
30 Keitel, David
31 Lackey, Benjamin
32 Logue, Joshua
33 Mohapatra, Satyanarayan
34 Piergiovanni, Francesco
35 Privitera, Stephen
36 Prix, Reinhard
37 Purrer, Michael
38 Re, Virginia
39 Serafinelli, Roberto
40 Wade, Leslie
41 Wen, Linqing
42 Wette, Karl
43 Whelan, John
44 Palomba, C.
45 Prodi, G.
Grupo 1
 2
 3
 4
 5
 6
 7
 8
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24 DAS-CEA-INPE-MCTI-GOV-BR
25
26 DSE-ETE-INPE-MCTI-GOV-BR
Afiliação 1 INFN
 2 The Amaldi 10 Parallel Session C2 on gravitational wave (GW) search results, data analysis and parameter estimation included three lively sessions of lectures by 13 presenters, and 34 posters. The talks and posters covered a huge range of material, including results and analysis techniques for ground-based GW detectors, targeting anticipated signals from different astrophysical sources: compact binary inspiral, merger and ringdown; GW bursts from intermediate mass binary black hole mergers, cosmic string cusps, core-collapse supernovae, and other unmodeled sources; continuous waves from spinning neutron stars; and a stochastic GW background. There was considerable emphasis on Bayesian techniques for estimating the parameters of coalescing compact binary systems from the gravitational waveforms extracted from the data from the advanced detector network. This included methods to distinguish deviations of the signals from what is expected in the context of General Relativity
 3 Nikhef
 4 N. Copernicus Astronomical Center
 5 Carleton College Northfield
 6 Albert-Einstein-Institut
 7 NASA Goddard Space Flight Center
 8 University of Florida
 9 Albert-Einstein-Institut
10 Kyoto University
11 Universite Paris
12 Cardiff University
13 University of Birmingham
14 Nikhef
15 University of Wisconsin
16 Albert-Einstein-Institut
17 Washington State University
18 University of the Balearic
19 Madingley Road Cambridge
20 University of Maryland
21 University of Massachusetts
22 University of Rome “Sapienza”
23 European Gravitational Observatory (EGO)
24 Instituto Nacional de Pesquisas Espaciais (INPE)
25 Albert-Einstein-Institut
26 Instituto Nacional de Pesquisas Espaciais (INPE)
27 Albert-Einstein-Institut
28 Tata Institute for Fundamental Research
29 Cardiff University School of Physics and Astronomy
30 Albert-Einstein-Institut
31 Princeton University
32 University of Glasgow
33 Syracuse University
34 INFN
35 California Institute of Technology
36 Albert-Einstein-Institut
37 Cardiff University
38 Universitá di Roma Tor Vergata
39 University of Rome “Sapienza”
40 University of Wisconsin
41 University of Western Australia
42 Albert-Einstein-Institut
43 Rochester Institute of Technology
44 INFN
45 INFN
Endereço de e-Mail do Autor 1
 2 ajw@catech.edu
 3
 4
 5
 6
 7
 8
 9
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24 filipe.davilsa@inpe.br
25
26 edgard.inpe@gmail.com
TítuloGravitational waves: search results, data analysis and parameter estimation: Amaldi 10 Parallel session C2
RevistaGeneral Relativity and Gravitation
Ano2015
Volume47
Número2
Palavras-ChaveCompact binary merger, Gravitational waves, Neutron stars, Parameter estimation, Stochastic background, Tests of general relativity.
ResumoThe Amaldi 10 Parallel Session C2 on gravitational wave (GW) search results, data analysis and parameter estimation included three lively sessions of lectures by 13 presenters, and 34 posters. The talks and posters covered a huge range of material, including results and analysis techniques for ground-based GW detectors, targeting anticipated signals from different astrophysical sources: compact binary inspiral, merger and ringdown; GW bursts from intermediate mass binary black hole mergers, cosmic string cusps, core-collapse supernovae, and other unmodeled sources; continuous waves from spinning neutron stars; and a stochastic GW background. There was considerable emphasis on Bayesian techniques for estimating the parameters of coalescing compact binary systems from the gravitational waveforms extracted from the data from the advanced detector network. This included methods to distinguish deviations of the signals from what is expected in the context of General Relativity.
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaB1_ASTRONOMIA_/_FÍSICA B1_MATEMÁTICA_/_PROBABILIDADE_E B1_QUÍMICA
Vinculação8JMKD3MGP7W/3F7TS9H
Tamanho227 KiB
Número de Arquivos1
Arquivo AlvoAstone_Gravitational.pdf
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Data de Acesso23 nov. 2020
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Área de identificação
Tipo da ReferênciaConference Proceedings
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W/3JJPL75
Repositóriosid.inpe.br/plutao/2015/06.01.14.11
Metadadossid.inpe.br/plutao/2015/06.01.14.11.37
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DOI10.3254/978-1-61499-476-3-321
Rótulolattes: 1448223845901360 2 NovaesWuenBernFerr:2015:LoPrNo
Chave de CitaçãoNovaesWuenBernFerr:2015:LoPrNo
TítuloLooking for primordial non-Gaussianity using Minkowski Functionals and Neural Networks
FormatoPapel
Ano2015
Data2014
Data de Acesso23 nov. 2020
Área de contextualização
Autor1 Novaes, Camila Paiva
2 Wuensche, Carlos Alexandre
3 Bernui, Armando
4 Ferreira, Ivan Soares
Grupo1 DAS-CEA-INPE-MCTI-GOV-BR
2 GB-GB-INPE-MCTI-GOV-BR
3 DAS-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)
Nome do EventoInternational School of Physics Enrico Fermi: New Horizons for Observational Cosmology
Localização do EventoBologna, Italia
Título do LivroProceedings
Editora (Publisher)IOS
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Área de conteúdo e estrutura
Estágio do Documentoconcluido
Estágio do Documentonot transferred
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Tipo do ConteudoExternal Contribution
Tipo SecundárioPRE CI
Tipo TerciárioPaper
Páginas321-326
Palavras-Chaveneural networks, minkowski functionals, non-gaussianity, Cosmology.
AreaCEA
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Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3KAAQRP
Repositóriosid.inpe.br/mtc-m21b/2015/09.23.12.53   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2015/09.23.12.53.01
Sitemtc-m21b.sid.inpe.br
DOI10.1007/s13538-015-0342-y
ISSN0103-9733
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoOjedaGonzalezDomiKaibPres:2015:OvImNu
Autor1 Ojeda Gonzalez, Arian
2 Domingues, Margarete Oliveira
3 Kaibara, M. K.
4 Prestes, Alan
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHQP
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 LAC-CTE-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 Universidade Federal Fluminense (UFF)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 arian.gonzalez@inpe.br
2 margarete.domingues@inpe.br
3
4 prestes@dge.inpe.br
TítuloGrad-shafranov reconstruction: overview and improvement of the numerical solution used in space physics
RevistaBrazilian Journal of Physics
Ano2015
Volume45
Número5
MêsOct.
Palavras-ChaveGrad-Shafranov equation, Magnetic flux-ropes, Cauchy problem, Space plasmas, Kinetic theory.
ResumoThe Grad-Shafranov equation is a Poisson's equation, i.e., a partial differential equation of elliptic type. The problem is depending on the initial condition and can be treated as a Cauchy problem. Although it is ill-posed or ill-conditioned, it can be integrated numerically. In the integration of the GS equation, singularities with large values of the potential arise after a certain number of integration steps away from the original data line, and a filter should be used. The Grad-Shafranov reconstruction (GSR) technique was developed from 1996 to 2000 for recovering two-dimensional structures in the magnetopause in an ideal MHD formulation. Other works have used the GSR techniques to study magnetic flux ropes in the solar wind and in the magnetotail from a single spacecraft dataset; posteriorly, it was extended to treat measurements from multiple satellites. From Vlasov equation, it is possible to arrive at the GS-equation in function of the normalized vector potential. A general solution is obtained using complex variable theory. A specific solution was chosen as benchmark case to solve numerically the GS equation. We propose some changes in the resolution scheme of the GS equation to improve the solution. The result of each method is compared with the solution proposed by Hau and Sonnerup (J. Geophys. Res. 104(A4), 6899-6917 (1999)). The main improvement found in the GS resolution was the need to filter B (x) values at each y value.
Páginas493-509
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PN
DivulgaçãoWEBSCI; PORTALCAPES; SCIELO; SCOPUS.
AreaCEA
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
Vinculação8JMKD3MGP7W/3DJMQKS
Tamanho1758 KiB
Número de Arquivos1
Arquivo Alvoojeda gonzalez_grad.pdf
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Data de Acesso23 nov. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3J7P6BE
Repositóriosid.inpe.br/mtc-m21b/2015/03.25.19.32
Metadadossid.inpe.br/mtc-m21b/2015/03.25.19.32.29
Sitemtc-m21b.sid.inpe.br
DOIdoi10.1002/2014JA020731
Rótuloself-archiving-INPE-MCTI-GOV-BR
ISSN0148-0227
2156-2202
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoPaulaJona:2015:LoScWe
Autor1 Paula, Eurico Rodrigues de
2 Jonah, O. F.
Identificador de Curriculo1 8JMKD3MGP5W/3C9JH2U
Grupo1 DAE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 eurico@dae.inpe.br
TítuloLow-latitude scintillation weakening during sudden stratospheric warming events
RevistaJournal of Geophysical Research
Ano2015
Volume120
Palavras-ChaveIonospheric scintillation, lunar tide effects over scintillation, vertical plasma drift, thermospheric wind.
ResumoGlobal Positioning System (GPS) L1-frequency (1.575 GHz) amplitude scintillations at São José dos Campos (23.1°S, 45.8°W, dip latitude 17.3°S), located under the southern crest of the equatorial ionization anomaly, are analyzed during the Northern Hemisphere winter sudden stratospheric warming (SSW) events of 2001/2002, 2002/2003, and 2012/2013. The events occurred during a period when moderate to strong scintillations are normally observed in the Brazilian longitude sector. The selected SSW events were of moderate and major categories and under low Kp conditions. The most important result of the current study is the long-lasting (many weeks) weakening of scintillation amplitudes at this low-latitude station, compared to their pre-SSW periods. Ionosonde-derived evening vertical plasma drifts and meridional neutral wind effects inferred from total electron content measurements are consistent with the observed weakening of GPS scintillations during these SSW events. This work provides strong evidence of SSW effects on ionospheric scintillations and the potential consequences of such SSW events on Global Navigation Satellite System-based applications.
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; AGU; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaA1_INTERDISCIPLINAR A1_GEOGRAFIA A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_CIÊNCIAS_AMBIENTAIS A1_CIÊNCIAS_AGRÁRIAS_I A2_QUÍMICA A2_ENGENHARIAS_IV A2_ENGENHARIAS_II A2_ENGENHARIAS_I A2_BIODIVERSIDADE B1_MATERIAIS B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_CIÊNCIA_DA_COMPUTAÇÃO B1_ASTRONOMIA_/_FÍSICA B2_PLANEJAMENTO_URBANO_E_REGIONAL_/_DEMOGRAFIA
Vinculação8JMKD3MGP7W/3DHJF42
Tamanho1934 KiB
Número de Arquivos1
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3KBEFLS
Repositóriosid.inpe.br/mtc-m21b/2015/09.30.12.31   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2015/09.30.12.31.01
Sitemtc-m21b.sid.inpe.br
DOI10.1016/j.newast.2015.06.001
ISSN1384-1076
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoPereiraMira:2015:RoDaMa
Autor1 Pereira, Eduardo dos Santos
2 Miranda, Oswaldo Duarte
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JJ2G
Grupo1 DAS-CEA-INPE-MCTI-GOV-BR
2 DAS-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 eduardo.pereira@inpe.br
2 oswaldo.miranda@inpe.br
TítuloThe role of the dark matter haloes on the cosmic star formation rate
RevistaNew Astronomy
Ano2015
Volume41
MêsNov.
Palavras-Chave(Cosmology):dark matter, Stars: formation, Stars: general, Galaxies: star formation.
ResumoThe cosmic star formation rate (CSFR) represents the fraction of gas that is converted into stars within a certain comoving volume and at a given time t. However the evolution of the dark matter haloes and its relationship with the CSFR is not yet clear. In this context, we have investigated the role of the dark halo mass function - DHMF - in the process of gas conversion into stars. We observed a strong dependence between the fraction of baryons in structures, fb, and the specific mass function used for describing the dark matter haloes. In some cases, we have obtained fb greater than one at redshift z=0. This result indicates that the evolution of dark matter, described by the specific DHMF, could not trace the baryonic matter without a bias parameter. We also observed that the characteristic time-scale for star formation, τ, is strongly dependent on the considered DHMF, when the model is confronted against the observational data. Also, as part of this work it was released, under GNU general public license, a Python package called pycosmicstar to study the CSFR and its relationship with the DHMF.
Páginas48-52
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Tamanho715 KiB
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Identificador8JMKD3MGP3W34P/3JLDG5P
Repositóriosid.inpe.br/mtc-m21b/2015/06.11.13.56
Metadadossid.inpe.br/mtc-m21b/2015/06.11.13.56.44
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DOI10.1088/0004-637X/804/1/33
ISSN0004-637X
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoSkowronSUHSSGPSJBBSKPSPKPUWABBBFFFILKMMMNOPRSSSTYMKFABCCDGHHJJLMNNPPYABBBCCCCCDDFGKKKMMMPRSWWWTBHHSSABBNDDDFGHHHHJKLLLMMPRRSSSSTW:2015:JoMiPl
Autor  1 Skowron, J.
  2 Shin, I-G.
  3 Udalski, A.
  4 Han, C.
  5 Sumi, T.
  6 Shvartzvald, Y.
  7 Gould, A.
  8 Prester, D. Dominis
  9 Street, R. A.
 10 Jorgensen, U. G.
 11 Bennett, D. P.
 12 Bozza, V.
 13 Szymanski, M. K.
 14 Kubiak, M.
 15 Pietrzynski, G.
 16 Soszynski, I.
 17 Poleski, R.
 18 Kozlowski, S.
 19 Pietrukowicz, P.
 20 Ulaczyk, K.
 21 Wyrzykowski, L.
 22 Abe, F.
 23 Bhattacharya, A.
 24 Bond, I. A.
 25 Botzler, C. S.
 26 Freeman, M.
 27 Fukui, A.
 28 Fukunaga, D.
 29 Itow, Y.
 30 Ling, C. H.
 31 Koshimoto, N.
 32 Masuda, K.
 33 Matsubara, Y.
 34 Muraki, Y.
 35 Namba, S.
 36 Ohnishi, K.
 37 Philpott, L. C.
 38 Rattenbury, N.
 39 Saito, T.
 40 Sullivan, D. J.
 41 Suzuki, D.
 42 Tristam, P. J.
 43 Yock, P. C. M.
 44 Maoz, D.
 45 Kaspi, S.
 46 Friedmann, M.
 47 Almeida, Leonardo Andrade de
 48 Batista, V.
 49 Christie, G.
 50 Choi, J. Y.
 51 DePoy, D. L.
 52 Gaudi, B. S.
 53 Henderson, C.
 54 Hwang, K. H.
 55 Jablonski, Francisco José
 56 Jung, Y. K.
 57 Lee, C. U.
 58 McCormick, J.
 59 Natusch, T.
 60 Ngan, H.
 61 Park, H.
 62 Pogge, R. W.
 63 Yee, J. C.
 64 Albrow, M. D.
 65 Bachelet, E.
 66 Beaulieu, J. P.
 67 Brillant, S.
 68 Caldwell, J. A. R.
 69 Cassan, A.
 70 Cole, A.
 71 Corrales, E.
 72 Coutures, Ch.
 73 Dieters, S.
 74 Donatowicz, J.
 75 Fouqué, P.
 76 Greenhill, J.
 77 Kains, N.
 78 Kane, S. R.
 79 Kubas, D.
 80 Marquette, J. B.
 81 Martin, R.
 82 Menzies, J.
 83 Pollard, K. R.
 84 Ranc, C.
 85 Sahu, K. C.
 86 Wambganss, J.
 87 Williams, A.
 88 Wouters, D.
 89 Tsapras, Y.
 90 Bramich, D. M.
 91 Horne, K.
 92 Hundertmark, M.
 93 Snodgrass, C.
 94 Steele, I. A.
 95 Alsubai, K. A.
 96 Browne, P.
 97 Burgdorf, M. J.
 98 Novati, S. Calchi
 99 Dodds, P.
100 Dominik, M.
101 Dreizler, S.
102 Fang, X. S.
103 Gu, C. H.
104 Hardis
105 Harpsoe, K.
106 Hessman, F. V.
107 Hinse, T. C.
108 Hornstrup, A.
109 Jessen-Hansen, J.
110 Kerins, E.
111 Liebig, C.
112 Lund, M.
113 Lundkvist, M.
114 Mancini, L.
115 Mathiasen, M.
116 Penny, M. T.
117 Rahvar, S.
118 Ricci, D.
119 Scarpetta, G.
120 Skottfelt, J.
121 Southworth, J.
122 Surdej, J.
123 Tregolan-Reed, J.
124 Wertz, O.
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 55 DAS-CEA-INPE-MCTI-GOV-BR
Afiliação  1 Warsaw University Observatory
  2 Chungbuk National University
  3 Warsaw University Observatory
  4 Chungbuk National University
  5 Osaka University
  6 Tel-Aviv University
  7 Ohio State University
  8 University of Rijeka
  9 Las Cumbres Observatory Global Telescope Network
 10 University of Copenhagen
 11 University of Notre Dame
 12 Università degli Studi di Salerno
 13 Warsaw University Observatory
 14 Warsaw University Observatory
 15 Warsaw University Observatory
 16 Warsaw University Observatory
 17 Warsaw University Observatory
 18 Warsaw University Observatory
 19 Warsaw University Observatory
 20 Warsaw University Observatory
 21 University of Cambridge
 22 Nagoya University
 23 University of Notre Dame
 24 Massey University
 25 University of Auckland
 26 University of Auckland
 27 National Astronomical Observatory of Japan
 28 Nagoya University
 29 Nagoya University
 30 Massey University
 31 Osaka University
 32 Nagoya University
 33 Nagoya University
 34 Konan University
 35 Osaka University
 36 Nagano National College of Technology
 37 University of British Columbia
 38 University of Auckland
 39 Tokyo Metropolitan College of Industrial Technology
 40 Victoria University
 41 Osaka University
 42 Victoria University
 43 University of Auckland
 44 Tel-Aviv University
 45 Tel-Aviv University
 46 Tel-Aviv University
 47 Instituto Nacional de Pesquisas Espaciais (INPE)
 48 Ohio State University
 49 Auckland Observatory
 50 Chungbuk National University
 51 Texas A&M University College Station
 52 Ohio State University
 53 Ohio State University
 54 Chungbuk National University
 55 Instituto Nacional de Pesquisas Espaciais (INPE)
 56 Chungbuk National University
 57 Korea Astronomy and Space Science Institute
 58 Centre for Backyard Astrophysics
 59 Auckland Observatory
 60 Auckland Observatory
 61 Chungbuk National University
 62 Ohio State University
 63 Ohio State University
 64 University of Canterbury
 65 Université de Toulouse
 66 Institut d’Astrophysique de Paris
 67 European Southern Observatory (ESO)
 68 McDonald Observatory
 69 Institut d’Astrophysique de Paris
 70 University of Tasmania
 71 Institut d’Astrophysique de Paris
 72 Institut d’Astrophysique de Paris
 73 Université de Toulouse
 74 Technical University of Vienna
 75 Université de Toulouse
 76 University of Tasmania
 77 European Southern Observatory
 78 NASA Exoplanet Science Institute
 79 Institut d’Astrophysique de Paris
 80 Institut d’Astrophysique de Paris
 81 Perth Observatory
 82 South African Astronomical Observatory
 83 University of Canterbury
 84 Institut d’Astrophysique de Paris
 85 Space Telescope Science Institute
 86 Zentrum für Astronomie der Universität Heidelberg (ZAH)
 87 Zentrum für Astronomie der Universität Heidelberg (ZAH)
 88 Institut d’Astrophysique de Paris
 89 Las Cumbres Observatory Global Telescope Network
 90 Qatar Foundation
 91 University of St Andrews
 92 University of St Andrews
 93 Max Planck Institute for Solar System Research
 94 Liverpool John Moores University
 95 Qatar Foundation
 96 University of St Andrews
 97 HE Space Operations GmbH
 98 NASA Exoplanet Science Institute
 99 University of St Andrews
100 University of St Andrews
101 Georg-August-Universität
102 Chinese Academy of Sciences
103 Chinese Academy of Sciences
104 University of Copenhagen
105 University of Copenhagen
106 Georg-August-Universität
107 Korea Astronomy and Space Science Institute
108 University of Manchester
109 Aarhus University
110 University of Manchester
111 University of St Andrews
112 Aarhus University
113 Aarhus University
114 Max Planck Institute for Astronomy
115 University of Copenhagen
116 University of Manchester
117 Sharif University of Technology
118 Institut d’Astrophysique et de Géophysique
119 Università degli Studi di Salerno
120 University of Copenhagen
121 Keele University
122 Institut d’Astrophysique et de Géophysique
123 NASA Ames Research Center
124 NASA Ames Research Center
Endereço de e-Mail do Autor  1
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 47 leonardo@das.inpe.br
 48
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 55 chico@das.inpe.br
TítuloOGLE-2011-BLG-0265Lb: a jovian microlensing planet orbiting an M DWARF
RevistaThe Astrophysical Journal
Ano2015
Volume804
Número33
Palavras-Chavegravitational lensing: micro – planetary systems.
ResumoWe report the discovery of a Jupiter-mass planet orbiting an M-dwarf star that gave rise to the microlensing event OGLE-2011-BLG-0265. Such a system is very rare among known planetary systems and thus the discovery is important for theoretical studies of planetary formation and evolution. High-cadence temporal coverage of the planetary signal, combined with extended observations throughout the event, allows us to accurately model the observed light curve. However, the final microlensing solution remains degenerate, yielding two possible configurations of the planet and the host star. In the case of the preferred solution, the mass of the planet is M M p J = +- 0.9 0.3 , and the planet is orbiting a star with a mass M M = +- 0.22 0.06 M.The second possible configuration (2σ away) consists of a planet with M M p J = +- 0.6 0.3 and host star with M M = +- 0.14 0.06 M. The system is located in the Galactic disk 34 kpc toward the Galactic bulge. In both cases, with an orbit size of 1.52.0 AU, the planet is a cold Jupiterlocated well beyond the snow line of the host star. Currently available data make the secure selection of the correct solution difficult, but there are prospects for lifting the degeneracy with additional follow-up observations in the future, when the lens and source star separate.
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
Vinculação8JMKD3MGP7W/3D7EQNH
Tamanho979 KiB
Número de Arquivos1
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3KAARRE
Repositóriosid.inpe.br/mtc-m21b/2015/09.23.13.05   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2015/09.23.13.05.23
Sitemtc-m21b.sid.inpe.br
DOI10.1007/s13538-015-0349-4
ISSN0103-9733
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoSouzaDomiMend:2015:EnSpPl
Autor1 Souza, Vitor Moura Cardoso e Silva
2 Domingues, Margarete Oliveira
3 Mendes Júnior, Odim
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHQP
3 8JMKD3MGP5W/3C9JJ28
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 LAC-CTE-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 vitor.souza@inpe.br
2 margarete.domingues@inpe.br
3 odim.mendes@inpe.br
TítuloEnhancement of space plasma images by complex wavelets
RevistaBrazilian Journal of Physics
Ano2015
Volume45
Número5
MêsOct.
Palavras-ChaveSolar corona, Coronal mass ejections (CMEs), Complex wavelet transform.
ResumoThe Sun is a natural laboratory for plasma processes. A myriad of instruments aboard satellites and on ground record(ed) the plasma emission in different ranges of the electromagnetic spectrum to help understand such processes. In particular, in the outer part of the solar atmosphere, the solar corona, we can observe a multitude of electrodynamical phenomena. There, the faint corona emission and the associated dynamic plasma structures (e.g., coronal mass ejections-CMEs) recorded in white-light images can be used as basis for some insight of this physical scenario. In order to characterize the dynamics and morphology of such structures in a better way, it seems crucial that some features of those images should be enhanced. To deal with this need, a new approach using a complex wavelet transform methodology was developed. With the proposed methodology, we can highlight the plasma ejections improving the identification of those structures.
Páginas510-517
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PN
DivulgaçãoWEBSCI; PORTALCAPES; SCIELO; SCOPUS.
AreaCEA
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
Vinculação8JMKD3MGP3W34P/3J3GFGP
Tamanho711 KiB
Número de Arquivos1
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Data de Acesso23 nov. 2020
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3KBB7KE
Repositóriosid.inpe.br/mtc-m21b/2015/09.29.18.29
Metadadossid.inpe.br/mtc-m21b/2015/09.29.18.29.08
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Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoVieiraGDWEGCGCPBASCSSBDRMJDBSGK:2015:PrDeIN
Autor 1 Vieira, Luis Eduardo Antunes
 2 Gonzalez, Alícia Licia Clua
 3 Dal Lago, Alisson
 4 Wrasse, Cristiano Max
 5 Echer, Ezequiel
 6 Guarnieri, Fernando Luis
 7 Cardoso, Flávia Reis
 8 Guerrero, G.
 9 Costa, Joaquim Eduardo Rezende
10 Palacios, J.
11 Balmaceda, Laura Antonia
12 Alves, Livia Ribeiro
13 Silva, L. da
14 Costa, Lucas Lopes
15 Sampaio, Marcelo
16 Soares, M. C. Rabello
17 Barbosa, M.
18 Domingues, Margarete Oliveira
19 Rigozo, Nivaor Rodolfo
20 Mendes Júnior, Odim
21 Jauer, P.
22 Dallaqua, Renato Sérgio
23 Branco, Renato Henrique
24 Stekel, Tardelli Ronan Coelho
25 Gonzalez Alarcon, Walter Demétrio
26 Kabata, Wanderli
Identificador de Curriculo 1
 2
 3 8JMKD3MGP5W/3C9JGH3
 4
 5 8JMKD3MGP5W/3C9JH3D
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15 8JMKD3MGP5W/3C9JHP8
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20 8JMKD3MGP5W/3C9JJ28
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22 8JMKD3MGP5W/3C9JJ5K
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25 8JMKD3MGP5W/3C9JJC4
26 8JMKD3MGP5W/3C9JJC8
Grupo 1 DGE-CEA-INPE-MCTI-GOV-BR
 2
 3 DGE-CEA-INPE-MCTI-GOV-BR
 4 DAE-CEA-INPE-MCTI-GOV-BR
 5 DGE-CEA-INPE-MCTI-GOV-BR
 6 YYY-CEA-INPE-MCTI-GOV-BR
 7
 8
 9 DAS-CEA-INPE-MCTI-GOV-BR
10
11 GES-CEA-SPG-INPE-MCTI-GOV-BR
12 DGE-CEA-INPE-MCTI-GOV-BR
13
14 SGP-ETE-INPE-MCTI-GOV-BR
15 DGE-CEA-INPE-MCTI-GOV-BR
16
17
18 LAC-CTE-INPE-MCTI-GOV-BR
19 DGE-CEA-INPE-MCTI-GOV-BR
20 DGE-CEA-INPE-MCTI-GOV-BR
21
22 LAP-CTE-INPE-MCTI-GOV-BR
23 ETE-ETE-INPE-MCTI-GOV-BR
24 GES-CEA-SPG-INPE-MCTI-GOV-BR
25 DGE-CEA-INPE-MCTI-GOV-BR
26 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2
 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
 8
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13
14 Instituto Nacional de Pesquisas Espaciais (INPE)
15 Instituto Nacional de Pesquisas Espaciais (INPE)
16
17
18 Instituto Nacional de Pesquisas Espaciais (INPE)
19 Instituto Nacional de Pesquisas Espaciais (INPE)
20 Instituto Nacional de Pesquisas Espaciais (INPE)
21
22 Instituto Nacional de Pesquisas Espaciais (INPE)
23 Instituto Nacional de Pesquisas Espaciais (INPE)
24 Instituto Nacional de Pesquisas Espaciais (INPE)
25 Instituto Nacional de Pesquisas Espaciais (INPE)
26 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor 1 luis.vieira@inpe.br
 2
 3 alisson.dallago@inpe.br
 4 cristiano.wrasse@inpe.br
 5 eecher@dge.inpe.br
 6
 7 flavia.cardoso@inpe.br
 8
 9 joaquim.costa@inpe.br
10
11 laura.balmaceda@inpe.br
12 livia.alves@inpe.br
13
14 lucas.costa@inpe.br
15 marcelo.sampaio@inpe.br
16
17
18 margarete.domingues@inpe.br
19 nivaor.rigozo@inpe.br
20 odim.mendes@inpe.br
21
22 renato.dallaqua@inpe.br
23 renato.branco@inpe.br
24 tardelli.stekel@inpe.br
25 walter.alarcon@inpe.br
26 wanderli@dge.inpe.br
TítuloPreliminary design of the INPE's solar vector magnetograph
Nome do EventoInternational Astronomical Union Symposium (IAU)
Ano2015
Título do LivroProceedings
Palavras-ChaveSun: photosphere, magnetic fields, techniques: polarimetric.
ResumoWe describe the preliminary design of a magnetograph and visible-light imager instrument to study the solar dynamo processes through observations of the solar surface magnetic field distribution. The instrument will provide measurements of the vector magnetic field and of the line-of-sight velocity in the solar photosphere. As the magnetic field anchored at the solar surface produces most of the structures and energetic events in the upper solar atmosphere and significantly influences the heliosphere, the development of this instrument plays an important role in reaching the scientific goals of The Atmospheric and Space Science Coordination (CEA) at the Brazilian National Institute for Space Research (INPE). In particular, the CEAs space weather program will benefit most from the development of this technology. We expect that this project will be the starting point to establish a strong research program on Solar Physics in Brazil. Our main aim is acquiring progressively the know-how to build state-of-the-art solar vector magnetograph and visible-light imagers for space-based platforms to contribute to the efforts of the solar-terrestrial physics community to address the main unanswered questions on how our nearby Star works.
Tipo SecundárioPRE CI
AreaCEA
Vinculação8JMKD3MGP3W34P/3JA39H2
Tamanho120 KiB
Número de Arquivos1
Arquivo Alvovieira_preliminary.pdf
Última Atualização2015:09.29.18.30.12 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator
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2018-06-04 02:55:43 :: administrator -> simone :: 2015
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Data de Acesso23 nov. 2020
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