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9 referências encontradas buscando em 17 dentre 17 Arquivos.
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3ARN427
Repositóriodpi.inpe.br/plutao/2011/11.23.16.20.11
Última Atualização2012:06.14.12.06.33 (UTC) ana.silveira
Repositório de Metadadosdpi.inpe.br/plutao/2011/11.23.16.20.12
Última Atualização dos Metadados2018:06.05.00.01.32 (UTC) administrator
Rótulolattes: 6929200500721452 5 AlvesScGoRoCaPa:2011:StAnLo
Chave de CitaçãoAlvesScGoRoCaPa:2011:StAnLo
TítuloStudy of Antennas for a Low Cost Interferometer
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho316 KiB
2. Contextualização
Autor1 Alves, Dimas Irion
2 Schuch, Nelson Jorge
3 Gomes, Natanael Rodrigues
4 Rosa, Guilherme Simon da
5 Camponogara, Ândrei
6 Paulo, Cláudio Machado
Grupo1 CRS-CCR-INPE-MCT-BR
2 CRS-CCR-INPE-MCT-BR
3 CRS-CCR-INPE-MCT-BR
4
5 CRS-CCR-INPE-MCT-BR
6 CRS-CCR-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2
3
4
5 acamponogara@gmail.com
Endereço de e-Mailacamponogara@gmail.com
Nome do EventoTwelfth International Congress of the Brazilian Geophysical Society.
Localização do EventoRio de Janeiro
Data2011
Título do LivroAnais
Tipo TerciárioResumo Estendido
Histórico (UTC)2011-11-24 11:03:14 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011
2012-02-24 02:24:38 :: secretaria.cpa@dir.inpe.br -> ana.silveira :: 2011
2012-06-14 12:06:33 :: ana.silveira -> administrator :: 2011
2018-06-05 00:01:32 :: administrator -> ana.silveira :: 2011
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ResumoThe project of a modern interferometric array similar to the Low Frequency Array (LOFAR) Prototype Station (LOPES), to cover the LOFAR frequency range under 100 MHz is being developed at the Southern Space Observatory (SSO, 29.4o S, 59.4o W), Sao Martinho da Serra, RS, Brazil. Therefore, it is necessary to study different kinds of antennas that cover the large proportions of the interferometer necessity. The large number of antennas required for a LOFAR like interferometer suggests that the antenna design must have: a low development cost, avoid complex mechanical structures, robust mechanical facilities, and a large useful bandwidth dominated by the Galactic radio noise, in order to maintain a low station cost. This work presents a study of four kinds of antennas designs (NLTA, Inverted-V dipole, Fork and Half-wavelength dipole), the results of antennas simulations comparisons using the NEC-2 software and finally for each antenna a cost-benefit analysis.
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URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/3ARN427
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Arquivo AlvoResumo Expandido CISBGF - Dimas Irion Alves - Março 2011 (2).pdf
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Unidades Imediatamente Superiores8JMKD3MGPCW/3EUFCFP
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3ASH2FH
Repositóriosid.inpe.br/mtc-m19/2011/11.28.16.19   (acesso restrito)
Última Atualização2011:11.28.16.22.16 (UTC) ana.silveira
Repositório de Metadadossid.inpe.br/mtc-m19/2011/11.28.16.19.19
Última Atualização dos Metadados2021:02.11.18.18.28 (UTC) administrator
Chave de CitaçãoBohrerSDCBAFABJ:2011:BrNACu
TítuloThe Brazilian NANOSATC-BR CubeSat
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho1271 KiB
2. Contextualização
Autor 1 Bohrer, Rubens Zolar Gehlen
 2 Schuch, Nelson Jorge
 3 Durão, Otávio Santos Cupertino
 4 Costa, Lucas L.
 5 Bürger, Eduardo E.
 6 Alves, Fernando L.
 7 Franke, Lucas L. C.
 8 Alves, Fernando L.
 9 Balestrin, Maurício R.
10 Jaenisch, Guilherme P.
Identificador de Curriculo 1
 2 8JMKD3MGP5W/3C9JHUD
 3 8JMKD3MGP5W/3C9JJ2L
Grupo 1 CRS-CCR-INPE-MCT-BR
 2 CRS-CCR-INPE-MCT-BR
 3 DMC-ETE-INPE-MCT-BR
 4 CRS-CCR-INPE-MCT-BR
 5
 6 CRS-CCR-INPE-MCT-BR
 7 CRS-CCR-INPE-MCT-BR
 8 CRS-CCR-INPE-MCT-BR
 9 CRS-CCR-INPE-MCT-BR
10 CRS-CCR-INPE-MCT-BR
Afiliação 1 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 National Institute for Space Research, São José dos Campos, SP, Brazil.
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoPico and Nano Satellite Workshop “Technology for Small Satellite Research”
Localização do EventoGermany
Data22-23 September
Tipo TerciárioSessão Oral
Histórico (UTC)2011-11-28 16:22:33 :: ana.silveira -> administrator :: 2011
2012-07-15 22:05:02 :: administrator -> ana.silveira :: 2011
2013-01-17 11:22:49 :: ana.silveira -> administrator :: 2011
2021-02-11 18:18:28 :: administrator -> ana.silveira :: 2011
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Palavras-ChaveNANOSATC-BR
anosatellite
ResumoThe Project NANOSATC-BR CubeSat Development consists the Brazilian, National Institute for Space Research and Federal University of Santa Maria, INPE-UFSM, Capacity Building program on space, engineering and computing sciences through a CubeSat program. The NANOSATC-BR1 nanosatellite is planned to be launch in a polar orbit inclined about 98° with respect to the Earths equatorial plane, at an approximate altitude of 650 km, with both objectives: to monitor the Geomagnetic field and its effects over the Brazilian territory, especially over the region knows as the South Atlantic Magnetic Anomaly (SAMA), using an off-the-shelf magnetic field sensor; and to capacity a new generation of scientists, engineers and researches, providing hands-on training and learning with aerospace technologies and Space Weather issues. In order to accomplish these aims, two 1U-CubeSat platforms: a Flight Model (FM) and an Engineering Model (EM); and a Small Satellite Ground Station, equipped with VHF/UHF band and S-band antennas, which will be installed in Santa Maria, South of Brazil, on the building of the Southern Regional Space Research Center, CRS/CCR/INPEMCT, INPEs sub-unit, have been purchased from the Dutch ISIS Company. With the delivery of the models and Ground Station in July 2011 and launch planned for later 2012, at the present moment, documentations, tests plans and specifications are under development. Undergraduate and Graduate students from UFSM, and Master and Doctored students from INPE are involved in different areas of the Project, covering mechanical analysis, test and integration documentations, even developments for new equipment, interfaces and software to be applied in the NANOSATC-BR1 mission. As a result, the NANOSATC-BR Project has been providing, to the Brazilian INPE-UFSM institutions, the development of CubeSats technologies, space knowledge, integration and tests procedures.
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Repositório Espelhosid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Unidades Imediatamente Superiores8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/446AF4B
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject targetfile tertiarymark type url volume
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3A5H85E
Repositóriosid.inpe.br/mtc-m19/2011/07.22.13.23   (acesso restrito)
Última Atualização2011:07.22.13.25.52 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2011/07.22.13.23.14
Última Atualização dos Metadados2018:06.05.04.24.36 (UTC) administrator
Chave de CitaçãoBremmSTGPFCSMP:2011:SeGeFi
TítuloSearch for geomagnetic field irregular pulsations in the South Atlantic magnetic anomaly region
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho320 KiB
2. Contextualização
Autor 1 Bremm, Tiago
 2 Schuch, Nelson Jorge
 3 Trivedi, Nalin Babulal
 4 Guimarães Dutra, Severino Luiz
 5 Pinheiro, Katia
 6 Fontes, Sérgio Luiz
 7 Coelho Stekel, Tardelli Ronan
 8 da Silva, Andirlei Claudir
 9 Marchezi, José Paulo
10 Piovesan, Talis
Identificador de Curriculo 1
 2 8JMKD3MGP5W/3C9JHUD
 3 8JMKD3MGP5W/3C9JHTS
 4 8JMKD3MGP5W/3C9JJ8J
Grupo 1 CRS-CCR-INPE-MCT-BR
 2 CRS-CCR-INPE-MCT-BR
 3 DGE-CEA-INPE-MCT-BR
 4 DGE-CEA-INPE-MCT-BR
 5
 6
 7
 8 CCR-CCR-INPE-MCT-BR
 9 CCR-CCR-INPE-MCT-BR
10 CRS-CCR-INPE-MCT-BR
Afiliação 1 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 National Observatory
 6 National Observatory
 7
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoMagnet Brazil, 1. Simpósio de Geomagnetismo do Brasil, 1.
Localização do EventoRio de Janeiro
Data5 a 10 junho de 2011
Tipo TerciárioPoster
Histórico (UTC)2011-07-22 13:25:52 :: ana.silveira -> administrator :: 2011
2018-06-05 04:24:36 :: administrator -> ana.silveira :: 2011
3. Conteúdo e estrutura
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Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-Chaveirregular pulsations
South Atlantic Magnetic Anomaly
ResumoThe present research aims to study the irregular pulsations in the geomagnetic field in the region of the South Atlantic Magnetic Anomaly (SAMA), with its center located near the Southern Space Observatory - OES/CRS/CCR/INPE-MCT, in São Martinho da Serra, RS, (29.42°S, 53.87°O, 480m a.s.l.). The irregular pulsations are geomagnetic pulsation of low frequency, produced mainly by charged particles beams that penetrate the high atmosphere. This injection of particles in the ionosphere causes the establishment of current systems, creating an increase in the conductivity of the ionosphere, which in turn provides a shield increasing hydro-magnetic waves excited by the beam, causing the irregular pulsation that occur in the early stages of the development of a Magnetic Storms. For the study of impulsive events at SAMA, measurements of the geomagnetic field are being made through a Fluxgate magnetometer, low-noise (0.1nT), three orthogonal components H (North - South), D (East - West) and Z (vertical), recording changes in magnetic field strength every three seconds. The data obtained at SSO are processed and studied at the Solar Physics, Interplanetary Medium and the Magnetosphere Laboratory in the Southern Regional Space Research Center - CRS/CCR/INPE-MCT, Santa Maria, RS, in cooperation with the National Observatory - ON/MCT. The analysis of these physical processes is important for the scientific community, facilitating the understanding of the processes occurring in the Earth's magnetosphere..
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Arquivo AlvoPowerPoint - Poster  Tiago Bremm (concluido).pdf
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Repositório Espelhosid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/3EUJHT5
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url versiontype volume
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3A5H9E2
Repositóriosid.inpe.br/mtc-m19/2011/07.22.13.39   (acesso restrito)
Última Atualização2011:07.22.13.42.46 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2011/07.22.13.39.57
Última Atualização dos Metadados2018:06.05.04.24.36 (UTC) administrator
Chave de CitaçãoMarcheziGuScTrSiCoAn:2011:LoPe1.
TítuloLong Periods (1.0 – 10 mhz) Geomagnetic Pulsations with Solar Cycle in the South Atlantic Magnetic Anomaly Region
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho340 KiB
2. Contextualização
Autor1 Marchezi, José Paulo
2 Guimarães Dutra, Severino Luiz
3 Schuch, Nelson Jorge
4 Trivedi, Nalin Babulal
5 Silva, Andirlei Claudir da
6 Coelho Stekel, Tardelli Roman
7 Antunes, Cassio Espindula
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JJ8J
3 8JMKD3MGP5W/3C9JHUD
4 8JMKD3MGP5W/3C9JHTS
Grupo1 CRS-CCR-INPE-MCT-BR
2 DGE-CEA-INPE-MCT-BR
3 CRS-CCR-INPE-MCT-BR
4
5 DGE-CEA-INPE-MCT-BR
6 CRS-CCR-INPE-MCT-BR
7 DGE-CEA-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoMagnet Brazil, 1. Simpósio de Geomagnetismo do Brasil, 1.
Localização do EventoRio de Janeiro
Data5 a 10 junho de 2011
Tipo TerciárioPoster
Histórico (UTC)2011-07-22 13:42:46 :: ana.silveira -> administrator :: 2011
2018-06-05 04:24:36 :: administrator -> ana.silveira :: 2011
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavecampo magnético
ResumoThe geomagnetic field is essential to the existence of life on the planet. The geomagnetic field acts as a barrier that protects the Earth from the high energy particles coming from the solar wind and outer space. The Earths magnetic Field undergoes changes on time scales of long or short periods, from seconds to several years (secular variations). The variations of about less than five years are of external origin, arising from the Sun-Earth interactions. The secular variations are associated with the processes within the Earth. The project is a study of the continuous pulsations Pc5 (150-600 seconds and frequency 2-7 millihertz), and its relation to solar cycle and the South Atlantic Magnetic Anomaly (SAMA). Region where the Earths magnetic field undergoes continuous slow decrease of its total field strength, caused by the westward drift of the SAMA center and the geomagnetic axis away from the anomaly region. The lower intensity of the geomagnetic field permits easier precipitation of charged particles in the atmosphere over the SAMA region. The SAMA center is located in the vicinity of the Southern Space Observatory SSO/CRS/CCR/INPE-MCT, in São Martinho da Serra, RS, Brazil (29.42° S, 53.82° W, elevation 488m). The geomagnetic pulsations are the result of the interactions between solar wind charged particles and the magnetospheric plasma in the terrestrial ionosphere. These variations are detected by fluxgate magnetometers (saturated nucleus) installed at the SSO.
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Arquivo AlvoPoster Abstract - -José Paulo Marchezi (concluido).pdf
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Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url volume
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/39UUFDS
Repositóriosid.inpe.br/mtc-m19/2011/06.30.12.31
Última Atualização2011:06.30.12.38.19 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2011/06.30.12.31.48
Última Atualização dos Metadados2018:06.05.04.24.29 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoPauloScAlViMoMo:2011:StIoCo
TítuloStudy of Ionospheric Cosmic Noise Absorption During a Complete Geomegnetic Storm on March, 2008
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho217 KiB
2. Contextualização
Autor1 Paulo, Cláudio Machado
2 Schuch, Nelson Jorge
3 Alves, Dimas Irion
4 Viera, Lucas Camponogara
5 Moro, Juliano
6 Moro, Pietro Fernando
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHUD
Grupo1
2 CRS-CCR-INPE-MCT-BR
Afiliação1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoMagnet Brazil 2011, 1.
Localização do EventoRio de Janeiro
Data5 a 10 junho de 2011
Tipo TerciárioPoster
Histórico (UTC)2011-07-22 13:59:07 :: ana.silveira -> administrator :: 2011
2018-06-05 04:24:29 :: administrator -> ana.silveira :: 2011
3. Conteúdo e estrutura
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Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavethe Ionospheric Cosmic Noise Absorption
Imaging Riometer for Ionospheric Studies (IRIS)
ResumoThe relation between geomagnetic storms that occurred from March 7 to 12, 2008 and the Ionospheric Cosmic Noise Absorption (ICNA) is presented. Data acquired by the Imaging Riometer for Ionospheric Studies (IRIS) and with a fluxgate Magnetometer, installed at the South Space Observatory (SSO/CRS/CCR/INPE - MCT, 29.4º S, 53.8º W, 480 m a.s.l.), São Martinho da Serra, RS, Brazil, under the South American Magnetic Anomaly (SAMA) was analyzed to study this moderate geomagnetic storm. The analysis was based on the geomagnetic indexes, like Dst and Kp, and with the variation of magnetic field components for the three phases of the storm: the storm sudden commencement, mean phase and recovery phase is presented. The analysis shows that during this geomagnetic storm the ICNA presents an increase positive variation.
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URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP7W/39UUFDS
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP7W/39UUFDS
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Arquivo AlvoMicrosoft PowerPoint - - I Magnet Brazil 2011 - Study of Ionospheric Cosmic Noise Absorption During a Complete Geomegnetic Storm on Mar.pdf
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3B7UKQL
Repositóriosid.inpe.br/mtc-m19/2012/01.19.12.57   (acesso restrito)
Última Atualização2012:01.19.13.01.26 (UTC) administrator
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Chave de CitaçãoPetryColpKato:2011:BaCoEs
TítuloBarometric Coefficients Estimation for Multi-directional Muon Detectors
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho43 KiB
2. Contextualização
Autor1 Petry, Adriano
2 Colpo, Miriam Pizzatto
3 Kato, Chihiro
Grupo1 CRS-CCR-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 adriano.petry@crs.inpe.br
2 miriamcolpo@msn.com
Nome do EventoConferência Latino-Americana de Geofísica Espacial, 9 (COLAGE).
Localização do EventoPuntarenas, Costa rica
Data5 A 10 april
Histórico (UTC)2012-01-19 13:01:27 :: ana.silveira -> administrator :: 2011
2018-06-05 04:25:25 :: administrator -> ana.silveira :: 2011
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Palavras-ChaveGlobal Muon Detector Network
ResumoThe Global Muon Detector Network (GMDN) provides important information that can be used in Space Weather forecasting. Coronal mass ejections (CMEs) may cause relevant variations in galactic cosmic rays (GCRs) intensities observed at the Earth, due to the formation of strong shock that travels slower that GCRs. This variation can be observed typically up to 4 hours ahead shock arrival. The National Institute for Space Research (INPE) participates in GMDN through a Multi-directional Muon Detector (MMD), operated at the Southern Space Observatory -SSO/CRS/INPE-MCT, in São Martinho da Serra, RS, Brazil. This detector measures secondary particles (muons) intensities at different directions, that are produced by interactions of primary GCRs with Earth´s upper atmosphere. However, muon counts can be affected also by environmental factors at the time of measure, like temperature and atmospheric pressure. The latter factor isone of the most relevant, and shows inversely proportional exponential relation to muon counting, i.e., the lower the pressure at the moment of measurement, higher muon counting is observed. In order to avoid the influence of barometric pressure, it is applied on every directional channel a different correction factor to the observed raw muon counts. A set of different barometric coefficients (betas) is used to calibrate muon counts measured by a MMD. So far, these values are calculated using a non-systematic semi-manual procedure, that may provide good estimatives, but does not guarantee the best possible values are obtained. In this work we propose an algorithm to automatically estimate the best possible values for barometric coefficients on every directional channel of a MMD. The proposed method initially discards all muon counts measured on days with sunspot number different from zero, in order to try to eliminate variations on countings due to solar activity. After that, the remaining counts are grouped by temperature step, so all measurements made at similar temperatures form a group where temperature influence is minimized. For each of these groups, the variance of muon counts related to barometric pressure is calculated. A high value of variance is desired for a group to be selected for beta estimation, since a more reliable linear regression can be applied. So, the winner group of measures that will be used in beta estimation will show simultaneously minimal influence on muons counts because of solar activity and temperature, and it will present muon counts well scattered along a wide range of atmospheric pressure values. Using those selected measures, the linear least squares method is applied and the angular coefficient from the best linear fit is calculated. At this moment, an angular coefficient equals to zero would indicate independence of muon counts due to atmospheric pressure variation. The raw muon counts are then calibrated using initially an arbitrary value of beta and the angular coefficient of best linear fit is calculated again. This step is repeated iteratively towards angular coefficient reduction, using different values of beta, until the angular coefficient value is zero. This algorithm was implemented computationally using Java programming language accessing a relational database, used to store and retrieve muon counts and environmental data, through Hibernate framework. Our approach was implemented and tested on MMD at SSO, showing relevant results that, for some directional channels, leaded to significantly different values when compared to the corresponding ones obtained using previous non-systematic procedure.
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Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject targetfile tertiarymark tertiarytype type url volume
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3B7ULSH
Repositóriosid.inpe.br/mtc-m19/2012/01.19.13.10   (acesso restrito)
Última Atualização2012:01.19.13.11.02 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2012/01.19.13.10.03
Última Atualização dos Metadados2018:06.05.04.25.25 (UTC) administrator
Chave de CitaçãoPetryVelSouPerBai:2011:AdSUCo
TítuloAdaptation of SUPIM code to operational ionospheric dynamics prediction in Brazilian Space Program
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho44 KiB
2. Contextualização
Autor1 Petry, Adriano
2 Velho, Haroldo Fraga de Campos
3 Souza, Jonas Rodrigues de
4 Pereira, André Grahal
5 Bailey, Graham John
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHC3
3 8JMKD3MGP5W/3C9JHFE
Grupo1 CRS-CCR-INPE-MCT-BR
2 LAC-CTE-INPE-MCT-BR
3 DAE-CEA-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoConferência Latino-Americana de Geofísica Espacial, 9 (COLAGE).
Localização do EventoPuntarenas, Costa rica
Data5 A 10 april
Histórico (UTC)2012-01-19 13:11:02 :: ana.silveira -> administrator :: 2011
2018-06-05 04:25:25 :: administrator -> ana.silveira :: 2011
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ResumoThe development and preliminary results of operational ionosphere dynamics prediction system for the Brazilian Space Program are presented. The system is based on the Sheffield University Plasmasphere-Ionosphere Model (SUPIM), a physics-based model computer code describing the distribution of ionization within the Earth mid to equatorial latitude ionosphere and plasmasphere. This model solves coupled time-dependent equations of continuity, momentum and energy balance along magnetic field lines for six different ions (O+, H+, He+, N2+, O2+ and NO+) and the electrons. Several physical and chemical processes are considered, and the code inputs include the solar flux, the neutral atmosphere model, and the model of meridional and zonal wind velocities. Depending upon the inputs, the model can describe different solar cycle, seasonal, daily, and magnetic activity variations. SUPIM outputs are the ion and electron densities, temperatures, and field-aligned fluxes. These outputs are given discreetly in a 2 dimensional plane aligned with Earth magnetic field lines, with fixed magnetic longitude coordinate. The fieldlines cove red are defined by the ground station coordinates and a pre-defined range of altitude. The geographic location of simulated points is aligned with magnetic coordinates, instead of the geographic coordinates. The first adaptation applied to the code was the output mapping from magnetic coordinates to geographical coordinates. It was made referring to the Earth´s magnetic field as an eccentric dipole, using the approximation based on International Geomagnetic Reference Field. During the system operation, several ionospheric simulation runs are performed at different geographic longitudes. The original code would not be able to run all simulations serially in reasonable time. So, a parallel version for the code (P-SUPIM) was developed for enhancing the performance using a hybrid parallel approach, employing the Message Passing Interface (MPI) version 2 and Open Multi-Processing (OpenMP) standards. Actually, a better performance was obtained using simultaneously both strategies for the P-SUPIM instead of considering each approach alone. After preliminary tests, it was frequently observed code instability, when negative ion temperatures or concentrations prevented the code from continuing its processing. After a detailed analysis, it was verified that most of these problems occurred due to concentration estimation of simulation points located at high altitudes, typically over 4000 Km of altitude. To achieve convergence, an artificial exponential decay for ion concentration was used above mentioned altitudes. This approach shown no significant difference from original code output, but improved substantially the code stability, since the ion diffusion is inversely proportional to the collisions, then at high altitudes the density of the atmosphere is very low, therefore the collisions of some atoms or molecules reaches values very close to zero. In order to make operational system even more stable, the initial altitude and initial ion concentration values used on exponential decay equation are changed within pre-defined values, in a search for convergence. When all P-SUPIM runs end, a set of simulation points are available, but its geographic location (following magnetic coordinates) does not allow geographic map visualization. A data interpolation technique was developed to obtain the ion concentration values for neighborhood of simulated points, in homogeneous grid. The neighborhood range can be increased, so all points in homogeneous grid are achieved. For every point in that grid, a weighted mean based on simulated point distance is applied. The resulting interpolated data is recorded in a file format that can be used on a software tool for visualization of Earth science data. The final system operates automatically using a cluster composed of 20 nodes, with 2 dual core processors on each. Every day, P-SUPIM is executed for ground station longitudes of -85, -80, -75, -70, -65, -60, - 55, -50, -45, -40, -35 e -30 degrees, covering South America region. A tri-dimensional homogeneous grid containing ion concentrations is generated for every hour of simulated day, in a total of 24 files. Its spatial resolution is 2 degrees of latitude for 2 degrees of longitude for 10 Km of altitude. The vertical total electron content (VTEC) is calculated for the grids points, and plotted in a geographic map. The whole process runs every day and predicts the VTEC values for South America with almost 24 hours ahead.
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Unidades Imediatamente Superiores8JMKD3MGPCW/3ESGTTP
8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn keywords label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject targetfile tertiarymark tertiarytype type url volume
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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3A5DQNP
Repositóriosid.inpe.br/mtc-m19/2011/07.21.18.53   (acesso restrito)
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Chave de CitaçãoPiovesanSCGTJACDMB:2011:NaMaSy
TítuloThe nanosatc-br1 magnetometer systems
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho208 KiB
2. Contextualização
Autor 1 Piovesan, Tális
 2 Schuch, Nelson Jorge
 3 Cupertino Durão, Otávio Santos
 4 Guimarães Dutra, Severino Luiz
 5 Trivedi, Nalin Babulal
 6 Junior, Odim Mendes
 7 Antunes, Cássio Espindola
 8 Coelho Stekel, Tardelli Ronan
 9 Da Silva, Andirlei Claudir
10 Marchezi, José Paulo
11 Bremm, Tiago
Identificador de Curriculo 1
 2 8JMKD3MGP5W/3C9JHUD
 3 8JMKD3MGP5W/3C9JJ2L
 4 8JMKD3MGP5W/3C9JJ8J
 5 8JMKD3MGP5W/3C9JHTS
 6 8JMKD3MGP5W/3C9JJ28
Grupo 1
 2 CRS-CCR-INPE-MCT-BR
 3 DMC-ETE-INPE-MCT-BR
 4 DGE-CEA-INPE-MCT-BR
 5
 6 DGE-CEA-INPE-MCT-BR
Afiliação 1
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoMagnet Brazil, 1. Simpósio de Geomagnetismo do Brasil, 1.
Localização do EventoRio de Janeiro
Data5 a 10 junho de 2011
Tipo TerciárioPoster
Histórico (UTC)2011-07-22 13:54:55 :: ana.silveira -> administrator :: 2011
2021-02-11 18:18:14 :: administrator -> ana.silveira :: 2011
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Palavras-ChaveCubeSat scientific
ResumoThe Brazilian NANOSATC-BR1 is a CubeSat scientific satellite developed mainly by undergraduate students from the Federal University of Santa Maria UFSM, Santa Maria, Rio Grande do Sul RS, Brazil, which are allocated and are developing research projects at the Solar Physics, Interplanetary Medium and Magnetospheres Laboratory - LSFMIM, in the Southern Regional Space Research Center CRS/CCR/INPEMCT, Santa Maria, RS, Brazil, to monitor and to study the Geomagnetic field in the central region of the Rio Grande do Sul, the further south state of Brazil, which is under the influence of the South Atlantic Magnetic Anomaly - SAMA. The CubeSat has in its structure two magnetometers that are essential for the mission success. One aims to the satellite attitude control in its space orbit, which will be provide by ISL/ISIS Innovative Space Logistics BV, from The Netherlands, which will made measurements of three orthogonal components H (North - South), D (East - West) and Z (vertical). The analysis of these measurements and compare with the vectors of reference previously established the CubeSat microprocessor generates a rotation matrix, or Quaternions in order to rotate it until the measurements are equal to those of the reference. The other magnetometer, Brand Honeywell Model HMR2300 or 2003, with the operating range of -200uT to 200uT and 2% accuracy at 25 º C, quantifies the components H, D, Z at a rate programmable from 10 to 154 acquisitions per second that will be processed and analyzed at the LFSMIM Lab.
ÁreaCEA
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Repositório Espelhosid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/446AF4B
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url volume
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1. Identificação
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Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3ARN429
Repositóriodpi.inpe.br/plutao/2011/11.23.16.20.13
Última Atualização2018:08.24.16.26.42 (UTC) simone
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Rótulolattes: 9965250176476500 17 SchuchDLRTMDDNPGMRASGCBBFASMPACSH:2011:PrNACu
Chave de CitaçãoSchuchDLRTMDDNPGMRASGCBBFASMPACSH:2011:PrNACu
TítuloProgress in the NANOSATC-BR Cubesats Development
Ano2011
Data de Acesso25 abr. 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho107 KiB
2. Contextualização
Autor 1 Schuch, Nelson Jorge
 2 Durão, Otávio Santos Cupertino
 3 Loureiro, G.
 4 Rozenfeld, Pawel
 5 Trivedi, N. B.
 6 Mendes Junior, O.
 7 Dutra, S. G. L.
 8 Dal Lago, A.
 9 de Nardin, C. M.
10 Palerosi, A. C.
11 Gomes, Natanael Rodrigues
12 Martins, J. B. S.
13 Reis, R. A. L.
14 Antunes, C. E.
15 Stekel, T. R. C
16 Guareschi, W. N.
17 Costa, Lucas Lopes
18 Burguer, E. e
19 Bohrer, R. Z. G.
20 Franke, Lucas Lourencena Caldas
21 Alves, F. L.
22 da Silva, A. C.
23 Marchezi, J. P.
24 Piovesan, T.
25 Alves, Dimas Irion
26 Camponogara, Ândrei
27 Souza, M. R.
28 Hammerschmitt, B. K.
Grupo 1 CRS-CCR-INPE-MCT-BR
 2 CPA-CPA-INPE-MCT-BR
 3 LIT-LIT-INPE-MCT-BR
 4 CRC-CRC-INPE-MCT-BR
 5
 6
 7 DGE-CEA-INPE-MCT-BR
 8 DGE-CEA-INPE-MCT-BR
Afiliação 1 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
 6
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor 1
 2
 3
 4
 5
 6
 7
 8
 9
10
11
12
13
14
15
16
17 lucas.matusalem@gmail.com
18
19
20
21
22
23
24
25
26 acamponogara@gmail.com
Endereço de e-Maillucas.matusalem@gmail.com
Nome do Evento62nd International Astronautical Congress
Localização do EventoCape Town, South Africa
Data2011
Título do LivroProceedings
Tipo TerciárioPaper
Histórico (UTC)2011-11-24 11:03:14 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011
2012-02-24 02:24:38 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2018-08-24 16:26:17 :: administrator -> simone :: 2011
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2021-02-03 17:56:50 :: administrator -> simone :: 2011
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É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-ChaveDesenvolvimento de Engenharias-Tecnologias
CubeSats
ÁreaCEA
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Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
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sid.inpe.br/bibdigital/2013/10.19.00.29 1
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
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