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2 referências encontradas buscando em 15 dentre 15 sites.
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3MRK48S
Repositóriosid.inpe.br/mtc-m21b/2016/11.22.19.52   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2016/11.22.19.52.04
Sitemtc-m21b.sid.inpe.br
DOI10.1016/j.jastp.2016.10.005
ISSN1364-6826
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoEgitoAndrBati:2016:VeWiMo
Autor1 Egito, Fábio
2 Andrioli, Vânia de Fátima
3 Batista, Paulo Prado
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JJ3H
Grupo1
2 CEA-CEA-INPE-MCTI-GOV-BR
3 DAE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Universidade Federal do Oeste da Bahia (UFOB)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 fabio.egito@ufob.edu.br
2 vania.andrioli@inpe.br
3 paulo.batista@inpe.br
TítuloVertical winds and momentum fluxes due to equatorial planetary scale waves using all-sky meteor radar over Brazilian region
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Ano2016
Volume149
MêsNov.
Palavras-ChaveMeteor radar, Planetary scale waves, Vertical wind.
ResumoIn the equatorial region planetary scale waves play an important role transporting significant amount of energy and momentum through atmosphere. Quantifying the momentum transported by these waves and its effects on the mean flow is rather important. Direct estimates of the momentum flux transported by waves require horizontal and vertical wind measurements. Ground-based meteor radars have provided continuous and reliable measurements of the horizontal wind components in the Mesosphere and Lower Thermosphere (MLT) region and have contributed to improve our knowledge of the dynamics of this region. However, instrumental limitations hinder its use for measuring vertical winds and momentum fluxes. On the other hand, according to Babu et al (2012), all- sky meteor radars are able to infer tridimensional winds when using a large number of meteor echoes centered at the meteor ablation peak. Following this approach, we have used measurements performed by a Meteor Radar installed at São João do Cariri, Brazil (7.4°S; 36.5°W) in order to measure vertical winds and calculate the momentum flux transported by equatorial planetary scale waves. In order to evaluate the accuracy of vertical wind values we have performed several tests based on a simple model considering real meteor distributions and theoretical equations for the MLT winds motion. From our tests, we inferred that Brazilian meteor radar data can be used for this purpose with an accuracy of ~ 1.8 m/s. The results show that the vertical wind presents magnitudes of a few meters per second and occasionally reaches magnitudes around 10 m/s. Below 92 km the vertical wind is predominantly upward during the whole year and above exhibits a semi-annual oscillation with downward phase during the equinoxes. Variations associated to planetary scale waves in the vertical wind are also observed and some of them appear simultaneously in the zonal and meridional wind as well. Largest wave induced amplitudes in the vertical wind are found in the 34 d band, reaching up to 4 m/s. From the vertical and zonal wind measurements, we calculated the vertical transport of zonal momentum in the 34 d band and found it to be maximum near autumn equinox, when its value reaches almost 20 m2/s2, while minimum momentum flux is observed after the winter solstice.
Páginas108-119
Idiomaen
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS.
AreaCEA
Nota SecundáriaA1_ENGENHARIAS_I A2_GEOCIÊNCIAS A2_ENGENHARIAS_III B1_INTERDISCIPLINAR B1_ENGENHARIAS_IV B1_BIODIVERSIDADE B2_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
Tamanho2134 KiB
Número de Arquivos1
Arquivo Alvoegito_vertical.pdf
Última Atualização2016:11.22.19.52.03 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 simone
Última Atualização dos Metadados2018:06.04.02.41.21 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
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Tipo do ConteudoExternal Contribution
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Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EU2FR5
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2016-11-22 19:52:04 :: administrator -> simone :: 2016
2016-11-22 19:52:32 :: simone -> administrator :: 2016
2016-12-06 19:38:02 :: administrator -> simone :: 2016
2016-12-23 14:04:53 :: simone -> administrator :: 2016
2017-01-09 13:59:35 :: administrator -> simone :: 2016
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2018-06-04 02:41:21 :: administrator -> simone :: 2016
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
Data de Acesso19 out. 2020
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Tipo da ReferênciaJournal Article
Identificador8JMKD3MGP3W34P/3LRJ3EP
Repositóriosid.inpe.br/mtc-m21b/2016/06.09.12.26   (acesso restrito)
Metadadossid.inpe.br/mtc-m21b/2016/06.09.12.26.18
Sitemtc-m21b.sid.inpe.br
DOI10.1088/1742-6596/706/5/052001
ISSN1742-6588
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Chave de CitaçãoPenacchioniBragÁvilDAmi:2016:TePeIm
Autor1 Penacchioni, Ana Virgínia
2 Braga, João
3 Ávila, Manuel Antonio Castro
4 D'Amico, Flávio
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHEK
Grupo1 CEA-CEA-INPE-MCTI-GOV-BR
2 DAS-CEA-INPE-MCTI-GOV-BR
3 DAS-CEA-INPE-MCTI-GOV-BR
4 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)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 ana.penacchioni@inpe.br
2 joao.braga@inpe.br
3 manuel.castro@inpe.br
4 flavio.damico@inpe.br
TítuloTelescope performance and image simulations of the balloon-borne coded-mask protoMIRAX experiment
RevistaJournal of Physics: Conference Series
Ano2016
Volume706
Palavras-ChaveProtoMIRAX, Astronomy, X-ray astrophysics, Astrophysics, Balloon experiment.
ResumoIn this work we present the results of imaging simulations performed with the help of the GEANT4 package for the protoMIRAX hard X-ray balloon experiment. The instrumental background was simulated taking into account the various radiation components and their angular dependence, as well as a detailed mass model of the experiment. We modeled the meridian transits of the Crab Nebula and the Galactic Centre region during balloon flights in Brazil (∼−23° of latitude and an altitude of View the MathML source) and introduced the correspondent spectra as inputs to the imaging simulations. We present images of the Crab and of three sources in the Galactic Centre region: 1E 1740.72942, GRS 1758258 and GX 1+4. The results show that the protoMIRAX experiment is capable of making spectral and timing observations of bright hard X-ray sources as well as important imaging demonstrations that will contribute to the design of the MIRAX satellite mission.
Páginas052001
NotasInternational Workshop on Hadron Physics, 13
Idiomaen
Tipo de Trabalhoconference paper
Tipo SecundárioPRE PI
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
AreaCEA
Nota SecundáriaB2_INTERDISCIPLINAR B2_ENGENHARIAS_III B3_MEDICINA_II B3_GEOCIÊNCIAS B4_MATERIAIS B4_ENGENHARIAS_II B4_BIOTECNOLOGIA C_QUÍMICA C_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA C_ENGENHARIAS_IV C_ECONOMIA C_ASTRONOMIA_/_FÍSICA
Tamanho1765 KiB
Número de Arquivos1
Arquivo Alvopenacchioni_telescope.pdf
Última Atualização2016:06.09.12.29.28 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 simone
Última Atualização dos Metadados2018:06.04.02.40.54 sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 administrator {D 2016}
Estágio do Documentoconcluido
É a matriz ou uma cópia?é a matriz
Espelhourlib.net/www/2011/03.29.20.55
e-Mail (login)simone
Grupo de Usuáriosadministrator
simone
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
Tipo de Versãopublisher
Política de Arquivamentodenypublisher denyfinaldraft12
Permissão de Leituradeny from all and allow from 150.163
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EU2FR5
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 09/06/2016 09:26 1.0 KiB 
Histórico2016-06-09 12:29:28 :: simone -> administrator :: 2016
2016-07-04 12:30:02 :: administrator -> simone :: 2016
2016-12-21 12:53:19 :: simone -> administrator :: 2016
2018-06-04 02:40:54 :: administrator -> simone :: 2016
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
Data de Acesso19 out. 2020
atualizar 
similares