1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | mtc-m16.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 6qtX3pFwXQZ3r59YDa/GwAPA |
Repositório | sid.inpe.br/iris@1916/2005/06.21.17.56 (acesso restrito) |
Última Atualização | 2005:06.21.03.00.00 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/iris@1916/2005/06.21.17.56.32 |
Última Atualização dos Metadados | 2021:07.18.04.01.20 (UTC) administrator |
Chave Secundária | INPE-12632-PRE/7924 |
ISSN | 1364-6826 |
Chave de Citação | PugachevaGusJaySchSpj:2005:CuReRa |
Título | Cusp region radiation belts in the dayside magnetosphere |
Ano | 2005 |
Mês | Mar. |
Data de Acesso | 29 abr. 2024 |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 828 KiB |
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2. Contextualização | |
Autor | 1 Pugacheva, Galina Ivanovna 2 Gusev, A. A. 3 Jayanthi, Udaya Bhaskaram 4 Schuch, Nelson Jorge 5 Spjeldvik, W. N. |
Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JJAE 4 8JMKD3MGP5W/3C9JHUD |
Grupo | 1 RSU-INPE-MCT-BR 2 DAS-INPE-MCT-BR |
Afiliação | 1 Instituto Nacional Pesquisas Espaciais,Divisãon de Astrofisica(INPE, DAS 2 INPE, Unidad Reg Pesquisas Espacials, Santa Maria, RS BR-12201970 Brazil 3 Russian Acad Sci, Inst Space Res, Moscow, V71 Russia 4 Weber State Univ, Ogden, UT 84408 USA |
Revista | Journal of Atmospheric and Solar-Terrestrial Physics |
Volume | 67 |
Número | 5 |
Páginas | 479-487 |
Histórico (UTC) | 2006-03-07 16:29:31 :: sergio -> administrator :: 2006-09-28 22:29:51 :: administrator -> sergio :: 2008-01-07 12:52:51 :: sergio -> administrator :: 2021-07-18 04:01:20 :: administrator -> marciana :: 2005 |
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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 |
Palavras-Chave | magnetosphere cusp region trapped particles radiation belts FIELD PARTICLES ELECTRONS SHEET MODEL |
Resumo | The possibility of quasi-stable trapping of charged particles of hundreds keV-MeV energy on the front side Earth magnetosphere is explored in this article by numerical modeling of the single particle orbits in the geomagnetic field utilizing empirical Tsyganenko model. On the front side magnetosphere the remote equatorial magnetic field lines are compressed to balance the solar wind pressure and exhibit two minima in the geomagnetic field strength magnitude along the field line in high latitudes on both sides of the equator which results in stable confinement structures in the north or/and the south hemispheres, providing energetic particle trapping for times from several minutes to durations of seasonal scale. Simulation of the energetic proton orbits in magnetosphere passing through the regions of magnetic field minima with different disturbance level and the Earth's tilt shows when and where these trapped radiation zones could exist. It is noted that the existence of this adiabatic confinement zone depends on the tilt of the geomagnetic dipole axis to the Sun-Earth direction. As a result the northern polar cap (cusp) confinement zone appears only during a summer solstice and similarly the southern hemisphere capture zone appears during a winter solstice. During equinox the confinement zones exist in both hemispheres in the disturbed magnetospheric conditions, however, they are less pronounced. The zones are essentially restricted to the sunlit magnetosphere. They form a kind of cusp radiation belt, where a proton drifts with a period of several minutes, conserving its 1st and the 2nd adiabatic invariants. The latitudinal width of the belt is very thin, about 2-5 latitudinal degrees. The particle orbits passing through opposite off-equatorial field minimum reveal another effect: a bound of the geomagnetic equatorial plane on the day sector. These and other features of the confinement zones in the two minima off-equatorial magnetic field regions are discussed. (c) 2004 Elsevier Ltd. All rights reserved. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Cusp region radiation... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Cusp region radiation... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | não têm arquivos |
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4. Condições de acesso e uso | |
Idioma | en |
Arquivo Alvo | cusp.pdf |
Grupo de Usuários | administrator sergio |
Visibilidade | shown |
Detentor da Cópia | SID/SCD |
Política de Arquivamento | denypublisher denyfinaldraft24 |
Permissão de Leitura | deny from all and allow from 150.163 |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETR8EH 8JMKD3MGPCW/3EUFCFP |
Divulgação | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
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7. Controle da descrição | |
e-Mail (login) | marciana |
atualizar | |
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