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8 referências encontradas buscando em 15 dentre 15 sites.
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3N7RDJ8
Repositóriosid.inpe.br/mtc-m21b/2017/01.18.15.10
Metadadossid.inpe.br/mtc-m21b/2017/01.18.15.10.09
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Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoAlvesBarbSimõ:2016:PaSiWa
Autor1 Alves, Maria Virginia
2 Barbosa, Marcos Vinicius Grala
3 Simões Júnior, Fernando J. L.
Identificador de Curriculo1 8JMKD3MGP5W/3C9JHRS
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 GESAST-CEA-SPG-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Federal de Pelotas (UFPEL)
Endereço de e-Mail do Autor1 mvirginia.alves@inpe.br
2 marcos.barbosa@inpe.br
TítuloParticle-in-cell Simulations of Waves in a Plasma Described by Kappa Velocity Distribution as Observed in the Saturn´s Magnetosphere
Nome do EventoAGU Fall Meeting
Ano2016
Data12-16 dec.
Localização do EventoSan Francisco
ResumoObservations have shown that several regions in space plasmas exhibit non-Maxwellian distributions with high energy superthermal tails. Kappa velocity distribution functions can describe many of these regions and have been used since the 60s. They suit well to represent superthermal tails in solar wind as well as to obtain plasma parameters of plasma within planetary magnetospheres. A set of initial velocities following kappa distribution functions is used in KEMPO1 particle simulation code to analyze the normal modes of wave propagation. Initial conditions are determined using observed characteristics for Saturn´s magnetosphere. Two electron species with different temperatures and densities and ions as a third species are used. Each electron population is described by a different kappa index. Particular attention is given to perpendicular propagation, Bernstein modes, and parallel propagation, Langmuir and electron-acoustic modes. The dispersion relation for the Bernstein modes is strongly influenced by the shape of the velocity distribution and consequently by the value of kappa index. Simulation results are compared with numerical solutions of the dispersion relation obtained in the literature and they are in good agreement.
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Campos Vaziosaccessionnumber archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress rightsholder secondarydate secondarymark serieseditor session shorttitle sponsor subject targetfile tertiarytype type url versiontype volume
Data de Acesso19 out. 2020
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3M9Q7SE
Repositóriosid.inpe.br/mtc-m21b/2016/08.17.13.59
Metadadossid.inpe.br/mtc-m21b/2016/08.17.13.59.08
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoBalan:2016:ReDeUn
AutorBalan, Nalan
GrupoDGE-CEA-INPE-MCTI-GOV-BR
AfiliaçãoInstituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autorbalannanan@gmail.com
TítuloRecent developments in the understanding of the mechanisms of EIA under quiet and active conditions
Nome do EventoAnnual Meeting Asia Oceania Geosciences Society, 13 (AOGS)
Ano2016
Data31 July - 05 Aug.
Localização do EventoBeijing
ResumoThe equatorial ionization anomaly (EIA), the largest ionospheric feature that covers over half the global area in 24 hours, was discovered by Namba and Maida in 1939 and Appleton in 1946. It has an ionization trough around the equator, crests at ~±15° magnetic latitudes and a crest-to-trough ratio of approximately 1.6 during quiet daytime. Though several mechanisms were suggested, the equatorial plasma fountain mechanism involving the upward ExB drift due to eastward electric field and downward field aligned plasma diffusion due to gravity and plasma pressure gradient forces was found to be able to model and explain the EIA [Moffett and Hanson, 1965]. However, the easy-to-understand misinterpretations of the involved physics of the plasma fountain and formation of EIA created misunderstandings in the literature, which has lead to wrong explanations for the strong EIA observed during major daytime space weather events. In this talk we review the recent understanding of the mechanisms of the plasma fountain and formation of EIA and try to clear the misunderstandings through basic principles, observations and modeling under both quiet and active conditions.
Idiomaen
Tipo SecundárioPRE CI
AreaCEA
Última Atualização dos Metadados2018:06.04.02.41.02 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
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2018-06-04 02:41:02 :: administrator -> simone :: 2016
Campos Vaziosaccessionnumber archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
Data de Acesso19 out. 2020
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3M9Q88B
Repositóriosid.inpe.br/mtc-m21b/2016/08.17.14.03
Metadadossid.inpe.br/mtc-m21b/2016/08.17.14.03.07
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoBalanEbSkOmBaNa:2016:InFoSe
Autor1 Balan, Nalan
2 Ebihara, Yusuke
3 Skoug, R.
4 Omura, Yoshiharu
5 Batista, Inez Staciarini
6 Nakamura, Takuji
Identificador de Curriculo1
2
3
4
5 8JMKD3MGP5W/3C9JHDA
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2
3
4
5 DAE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Kyoto University
3 Los Alamos National Laboratory
4 Kyoto University
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 National Institute of Polar Research
Endereço de e-Mail do Autor1 balannanan@gmail.com
2
3
4
5 inez.batista@inpe.br
TítuloIndices for forecasting severe space weather
Nome do EventoAnnual Meeting Asia Oceania Geosciences Society, 13 (AOGS)
Ano2016
Data31 July - 05 Aug.
Localização do EventoBeijing
ResumoIndices for Forecasting Severe Space Weather Nanan BALAN1#+, Yusuke EBIHARA2, R. SKOUG3, Yoshiharu OMURA2, Inez BATISTA1, Takuji NAKAMURA4 1 National Institute for Space Research, Brazil, 2 Kyoto University, Japan, 3 Los Alamos National Laboratory, United States, 4 National Institute of Polar Research, Japan #Corresponding author: balannanan@gmail.com +Presenter We suggest indices for forecasting severe space weather (SvSW) at the Earth that can damage technological systems such as electric power grids for the first time using ACE and IMP satellite data and Dst index. We study the characteristics of the CMEs that produced all 90 intense geomagnetic storms (DstMin < -100 nT) including 2 SvSW events since 1998 and earlier SvSW events such as the Carrington event of 1859, Quebec event of 1989 and an event in 1958. The CME and IMF parameters corresponding to the main phase (MP) of the geomagnetic storms are used to develop a forecast scheme. The scheme is tested using hourly values of solar wind and IMF. The results reveal that (1) all known electric power outages happened during the SvSW events that produced extreme geomagnetic storms having high mean Dst during MP (mean DstMP < -250 nT). (2) The products (ΔV x Bz), (V x Bz) and (P x Bz) show very large negative values at the CME fronts (of velocity ΔV) that caused SvSW, with V, P and Bz being the solar wind velocity in km s-1, dynamic pressure in nPa and north-south (northward positive) component of IMF in nT. (3) The product (ΔV x Bz) seems a suitable index for forecasting SvSW.
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Tipo SecundárioPRE CI
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Última Atualização dos Metadados2018:06.04.02.41.02 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
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agreement.html 17/08/2016 11:03 1.0 KiB 
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2018-06-04 02:41:02 :: administrator -> simone :: 2016
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Data de Acesso19 out. 2020
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3LQKDJP
Repositóriosid.inpe.br/mtc-m21b/2016/06.03.16.20
Metadadossid.inpe.br/mtc-m21b/2016/06.03.16.20.56
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoChian:2016:MaCoSt
AutorChian, Abraham Chian-Long
GrupoDGE-CEA-INPE-MCTI-GOV-BR
AfiliaçãoInstituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autorachian@dge.inpe.br
TítuloMagnetic coherent structures in space plasmas
Nome do EventoChaotic Modeling and Simulation International Conference, 9 (CHAOS)
Ano2016
Data23-26 May
Localização do EventoLondon
Tipo SecundárioPRE CI
AreaCEA
Última Atualização dos Metadados2018:06.04.02.40.51 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
Estágio do Documentoconcluido
Espelhourlib.net/www/2011/03.29.20.55
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Grupo de Leitoresadministrator simone
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Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
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Permissão de Leituraallow from all
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agreement.html 03/06/2016 13:20 1.0 KiB 
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2018-06-04 02:40:51 :: administrator -> simone :: 2016
Campos Vaziosabstract accessionnumber archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
Data de Acesso19 out. 2020
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3LTD6UB
Repositóriosid.inpe.br/mtc-m21b/2016/06.20.17.03
Metadadossid.inpe.br/mtc-m21b/2016/06.20.17.03.14
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoChianMunoRemp:2016:EdChGe
Autor1 Chian, Abraham Chian-Long
2 Munoz, Pablo
3 Rempel, Erico Luiz
Grupo1
2
3 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Tecnológico de Aeronáutica (ITA)
2 Universidad de La Serena
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 abraham.chian@gmail.com
2 pablocus@gmail.com
3 erico_rempel@yahoo.com.br
TítuloEdge of chaos and genesis of turbulence
Nome do EventoInternational Conference on Nonlinear Science and Complexity, 6
Ano2016
Data16-20 May
Localização do EventoSão José dos Campos, SP
Palavras-ChaveEdge of chaos, chaotic saddle, turbulence, regularized long-wave equation, multistability.
ResumoThe edge of chaos is analyzed in a spatially extended system, modeled by the regularized long-wave equation, prior to the transition to permanent spatiotemporal chaos. In the presence of coexisting attractors, a chaotic saddle is born at the basin boundary due to a smooth-fractal metamorphosis. As a control parameter is varied, the chaotic transient evolves to well-developed transient turbulence via a cascade of fractal-fractal metamorphoses. The edge state responsible for the edge of chaos and the genesis of turbulence is an unstable traveling wave in the laboratory frame, corresponding to a saddle point lying at the basin boundary in the Fourier space.
Tipo SecundárioPRE CI
AreaCEA
Última Atualização dos Metadados2018:06.04.02.40.56 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
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Espelhourlib.net/www/2011/03.29.20.55
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Visibilidadeshown
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Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
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Permissão de Leituraallow from all
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
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agreement.html 20/06/2016 14:03 1.0 KiB 
Histórico2016-06-20 17:03:39 :: simone -> administrator :: 2016
2018-06-04 02:40:56 :: administrator -> simone :: 2016
Campos Vaziosaccessionnumber archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
Data de Acesso19 out. 2020
atualizar 
Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3LSN3NE
Repositóriosid.inpe.br/mtc-m21b/2016/06.16.13.59
Metadadossid.inpe.br/mtc-m21b/2016/06.16.13.59.39
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoChianRempSanj:2016:TrChCo
Autor1 Chian, Abraham Chian-Long
2 Rempel, Erico Luiz
3 Sanjuán, Miguel
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidad Rey Juan Carlos
Endereço de e-Mail do Autor1 abraham.chian@gmail.com
2 erico_rempel@yahoo.com.br
3 miguel.sanjuan@urjc.es
TítuloTransient chaos in complex systems
Nome do EventoInternational Conference on Nonlinear Science and Complexity, 6
Ano2016
Data16-20 May
Localização do EventoSão José dos Campos, SP
ResumoTransient chaos refers to chaotic phenomena that appear in a finite lifetime. In contrast to permanent chaos associated with the asymptotic state, transient chaos are associated with a nonequilibrium state that has different behavior from the asymptotic behavior of a system. Examples of complex phenomena and dynamical structures related to transient chaos are: chaotic saddles, chaotic leaking systems, crises, on-off intermittency, edge of chaos, chaotic advection, fractal basin boundaries, transport barriers, and turbulence. This mini-symposium aims to discuss the concepts and applications of transient chaos in astrophysics, biology, fluids, and plasmas.
Idiomaen
Tipo SecundárioPRE CI
AreaCEA
Última Atualização dos Metadados2018:06.04.02.40.56 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
Estágio do Documentoconcluido
Espelhourlib.net/www/2011/03.29.20.55
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Grupo de Leitoresadministrator
simone
Visibilidadeshown
Transferível1
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
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Estágio do Documentonot transferred
Permissão de Leituraallow from all
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
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Conteúdo da Pasta agreement
agreement.html 16/06/2016 10:59 1.0 KiB 
Histórico2016-06-16 17:08:25 :: simone -> administrator :: 2016
2016-06-20 11:25:45 :: administrator -> simone :: 2016
2016-06-20 15:50:13 :: simone -> administrator :: 2016
2018-06-04 02:40:56 :: administrator -> simone :: 2016
Campos Vaziosaccessionnumber archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
Data de Acesso19 out. 2020
atualizar 
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Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3LSNKAE
Repositóriosid.inpe.br/mtc-m21b/2016/06.16.17.08
Metadadossid.inpe.br/mtc-m21b/2016/06.16.17.08.24
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoChimanskiCherRemp:2016:RoHyIn
Autor1 Chimanski, E. V.
2 Chertovskih, R.
3 Rempel, Erico Luiz
Grupo1
2
3 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Tecnológico de Aeronáutica (ITA)
2 Instituto Tecnológico de Aeronáutica (ITA)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 kimor@ita.br
2 evchimanski@gmail.com
3 erico_rempel@yahoo.com.br
TítuloRoute to hyperchaos and intermittency in Rayleigh-Bernard Convection
Nome do EventoInternational Conference on Nonlinear Science and Complexity, 6
Ano2016
Data16-20 May
Localização do EventoSão José dos Campos, SP
Palavras-ChaveBifurcation, hyperchaos, chaotic saddle, intermittency, Rayleigh-Benard convection.
ResumoTransition to hyperchaotic regimes in Rayleigh-Benard convection in a square periodicity cell is studied by three-dimensional numerical simulations. By fixing the Prandtl number and varying the Rayleigh number as a control parameter, a bifurcation diagram is constructed where a route involving quasiperiodic regimes with two and three incommensurate frequencies, multistability, chaotic intermittent attractors and a sequence of boundary and interior crises is shown. The three largest Lyapunov exponents exhibit a linear scaling with the Rayleigh number and are positive in the final hyperchaotic attractor. Thus, a route to weak turbulence is found. R. Chertovskih, E.V. Chimanski, E.L. Rempel. Route to hyperchaos in Rayleigh-Benard convection. Europhysics Letters 112 (1), 14001 (2015) E. V. Chimanski, R. Chertovskih, E. L. Rempel. Intermittency route to hyperchaos in 3D RayleighBenard convection. Advances in Space Research, in press (2016).
Tipo SecundárioPRE CI
AreaCEA
Última Atualização dos Metadados2018:06.04.02.40.56 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
Estágio do Documentoconcluido
Espelhourlib.net/www/2011/03.29.20.55
e-Mail (login)simone
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Transferível1
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
Tipo do ConteudoExternal Contribution
Estágio do Documentonot transferred
Permissão de Leituraallow from all
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 16/06/2016 14:08 1.0 KiB 
Histórico2016-06-20 17:00:34 :: simone -> administrator :: 2016
2018-06-04 02:40:56 :: administrator -> simone :: 2016
Campos Vaziosaccessionnumber archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
Data de Acesso19 out. 2020
atualizar 
Tipo da ReferênciaConference Proceedings
Identificador8JMKD3MGP3W34P/3LTD7A8
Repositóriosid.inpe.br/mtc-m21b/2016/06.20.17.07
Metadadossid.inpe.br/mtc-m21b/2016/06.20.17.07.11
Sitemtc-m21b.sid.inpe.br
Chave SecundáriaINPE--PRE/
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoRempelMiraChia:2016:SuAmSy
Autor1 Rempel, Erico Luiz
2 Miranda, Rodrigo
3 Chian, Abraham Chian Long
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade de Brasília (UnB)
3 Instituto Tecnológico de Aeronáutica (ITA)
Endereço de e-Mail do Autor1 erico_rempel@yahoo.com.br
2 rmiracer@gmail.com
3 abraham.chian@gmail.com
TítuloSupertransient and amplitude-phase synchronization in a astrophysical shear flows
Nome do EventoInternational Conference on Nonlinear Science and Complexity, 6
Ano2016
Data16-20 May
Localização do EventoSão José dos Campos, SP
Palavras-ChaveOn-off intermittency, amplitude-phase synchronization, accretion discs, magnetohydrodynamics, turbulence.
ResumoWe study the development of coherent structures in local simulations of the magnetorotational instability in accretion discs in regimes of onoff intermittency. In Chian et al. (2010), we have shown that the laminar and bursty states due to the onoff spatiotemporal intermittency in a onedimensional model of non-linear waves correspond, respectively, to non- attracting coherent structures with higher and lower degrees of amplitude-phase synchronization. In this paper, we extend these results to a three-dimensional model of magnetized Keplerian shear flows. Keeping the kinetic Reynolds number and the magnetic Prandtl number fixed, we investigate two different intermittent regimes by varying the plasma beta parameter. The first regime is characterized by turbulent patterns interrupted by the recurrent emergence of a large-scale coherent structure known as two-channel flow, where the state of the system can be described by a single Fourier mode. The second regime is dominated by the turbulence with sporadic emergence of coherent structures with shapes that are reminiscent of a perturbed channel flow. By computing the Fourier power and phase spectral entropies in three dimensions, we show that the large-scale coherent structures are characterized by a high degree of amplitude-phase synchronization.
Tipo SecundárioPRE CI
AreaCEA
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Data de Acesso19 out. 2020
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