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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YDa/GwAPA
Repositóriosid.inpe.br/iris@1916/2005/06.21.17.56   (acesso restrito)
Última Atualização2005:06.21.03.00.00 (UTC) administrator
Repositório de Metadadossid.inpe.br/iris@1916/2005/06.21.17.56.32
Última Atualização dos Metadados2021:07.18.04.01.20 (UTC) administrator
Chave SecundáriaINPE-12632-PRE/7924
ISSN1364-6826
Chave de CitaçãoPugachevaGusJaySchSpj:2005:CuReRa
TítuloCusp region radiation belts in the dayside magnetosphere
Ano2005
MêsMar.
Data de Acesso29 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho828 KiB
2. Contextualização
Autor1 Pugacheva, Galina Ivanovna
2 Gusev, A. A.
3 Jayanthi, Udaya Bhaskaram
4 Schuch, Nelson Jorge
5 Spjeldvik, W. N.
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JJAE
4 8JMKD3MGP5W/3C9JHUD
Grupo1 RSU-INPE-MCT-BR
2 DAS-INPE-MCT-BR
Afiliação1 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
RevistaJournal of Atmospheric and Solar-Terrestrial Physics
Volume67
Número5
Páginas479-487
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
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-Chavemagnetosphere
cusp region
trapped particles
radiation belts FIELD
PARTICLES
ELECTRONS
SHEET
MODEL
ResumoThe 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.
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Arquivo Alvocusp.pdf
Grupo de Usuáriosadministrator
sergio
Visibilidadeshown
Detentor da CópiaSID/SCD
Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EUFCFP
DivulgaçãoWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2003/08.15.17.40
6. Notas
Campos Vaziosalternatejournal 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
7. Controle da descrição
e-Mail (login)marciana
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