1. Identificação | |
Tipo de Referência | Artigo em Evento (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/3QTFT62 |
Repositório | sid.inpe.br/mtc-m21c/2018/04.16.15.18 |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2018/04.16.15.18.39 |
Última Atualização dos Metadados | 2020:12.07.21.11.29 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
Chave de Citação | CarmoBeckCamaMoni:2018:CoDiTe |
Título | Comparison between different tec calculation techniques to characterize the ionosphere in the brazilian sector |
Ano | 2018 |
Data de Acesso | 12 maio 2024 |
Tipo Secundário | PRE CI |
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2. Contextualização | |
Autor | 1 Carmo, Carolina de Sousa do 2 Becker Guedes, Fábio 3 Camargo, P. O. 4 Monico, J. F. G. |
Grupo | 1 GES-CEA-SESPG-INPE-MCTIC-GOV-BR 2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Universidade Estadual Paulista (UNESP) 4 Universidade Estadual Paulista (UNESP) |
Endereço de e-Mail do Autor | 1 carolina.carmo@inpe.br 2 fabio.guedes@inpe.br |
Nome do Evento | Latin American Conference on Space Geophysics, 11 (COLAGE) |
Localização do Evento | Buenos Aires, Argentina |
Data | 16-20 abr. |
Histórico (UTC) | 2018-04-16 15:19:07 :: simone -> administrator :: 2018 2018-04-18 05:03:02 :: administrator -> administrator] :: 2018 2018-04-18 05:03:02 :: administrator] -> administrator :: 2018 2018-07-04 17:51:13 :: administrator -> simone :: 2018 2018-08-08 11:49:11 :: simone -> administrator :: 2018 2020-12-07 21:11:29 :: administrator -> simone :: 2018 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Resumo | The Total Electron Content (TEC) of the ionosphere can be calculated by parameters observed by GPS receivers located in the ground. As a result of the differential phase and group calculation, the non-dispersive terms are canceled, leaving terms due to biases of the satellites and the receiver together with the ionospheric error contribution to the signal. The slant TEC (STEC) corresponds to an arc of TEC for each satellite measured by a given receiver. The combination of the various STECs observed by a receiver using selected methods and mapping functions results in a vertical TEC (VTEC) over the ground station. In this work, the performance of three different VTEC calculation techniques, each one using their own methods to eliminate biases and to obtain VTEC from STECs, is evaluated to describe the ionosphere conditions in the equatorial and low latitude regions in the Brazilian sector. I order to do this, data from a station in the equatorial region, Sao Luis, and a station in the southern crest of the Equatorial Ionization Anomaly (EIA), Cachoeira Paulista, were used. The study was made for a period of minimum solar activity (November 2008 to October 2009) and one of maximum solar activity (November 2014 to October 2015) and the seasonality of TEC along the year was also studied. The three techniques used are: (I) the technique developed by the University of Nagoya, Japan, and adjusted at the National Institute of Space Research (INPE), Brazil, to be used by the Brazilian Space Weather Program (EMBRACE), (II) a technique developed at Boston College, USA, and (III) the method proposed by the International Centre for Theoretical Physics (ICTP), Italy. The evaluation of the TEC curves obtained showed that all three techniques present results consistent with each other but with some small divergences in certain periods. The three techniques show the significant reduction of the TEC in the period of minimum solar activity and during the winter in any condition of solar activity. All techniques showed an increase in TEC at the station under the crest of the EIA in the summer and during the equinoxes due to the intensification of the fountain effect during the day and the pre-reversion peak at the sunset. The large discrepancies between the results obtained by the three techniques were observed during the beginning of the night hours due to the presence of ionospheric irregularities. The method used in INPE responds well to the daily, seasonal and solar cycle variations of the TEC, presenting, on several occasions, intermediate results with respect to the other techniques in the Brazilian region, showing to be suitable to be used by EMBRACE program to monitoring this region. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Comparison between different... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Comparison between different... |
Conteúdo da Pasta doc | não têm arquivos |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Vinculação | 8JMKD3MGP3W34P/3QJNJHE |
Repositório Espelho | urlib.net/www/2011/03.29.20.55 |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETL868 8JMKD3MGPCW/3F2PBEE |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | 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 readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarytype type url versiontype volume |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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