| 1. Identificação | |
| Tipo de Referência | Artigo em Evento (Conference Proceedings) |
| Site | mtc-m16b.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Repositório | sid.inpe.br/mtc-m17@80/2007/12.17.14.15 |
| Repositório de Metadados | sid.inpe.br/mtc-m17@80/2007/12.17.14.15.17 |
| Última Atualização dos Metadados | 2018:06.05.03.36.36 (UTC) administrator |
| Chave Secundária | INPE--PRE/ |
| Chave de Citação | CardosoAlveViei:2007:AdDiTi |
| Título | Adding dipole tilt in a MHD two-dimensional code for studying magnetospheric configuration  |
| Ano | 2007 |
| Data de Acesso | 21 maio 2024 |
| Tipo Secundário | PRE CN |
| 2. Contextualização | |
| Autor | 1 Cardoso, Flávia Reis 2 Alves, Maria Virgínia 3 Vieira, Luis Eduardo A. |
| Grupo | 1 LAP-INPE-MCT-BR 2 LAP-INPE-MCT-BR |
| Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Max-Planck-Institute for Solar System Research |
| Nome do Evento | Encontro Brasileiro de Física dos Plasmas, 9. |
| Localização do Evento | São Pedro, SP |
| Data | 25-28 Nov. |
| Tipo Terciário | Poster |
| Histórico (UTC) | 2007-12-17 14:15:17 :: simone -> administrator :: 2012-10-24 00:13:41 :: administrator -> simone :: 2013-02-20 15:20:15 :: simone -> administrator :: 2007 2018-06-05 03:36:36 :: administrator -> marciana :: 2007 |
| 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 size of the magnetosphere is determined by the balance between the solar wind dynamic pressure and the pressure exerted by the magnetosphere. The shape of the magnetosphere is additionally in°uenced by the drag of the solar wind, or tangential stress, on it. This drag is predominantly caused by the mechanism known as magnetic reconnection in which the magnetic ¯eld of the solar wind links to the magnetic ¯eld of the magnetosphere. The interaction between the solar wind and planetary magnetospheres is not easily understood just from the measurements, limited by spacecrafts trajectories. The global magnetohydrodynamic model (MHD), developed to solve for the magnetospheric con¯guration and to provide a self-consistent picture of the solar wind-magnetosphere interaction process, has been successful used for the past decades. The MHD theory deals with the macroscopic energy conversion governing the global con¯guration, that is, the physical processes involved in the conversion among the magnetic, kinetic and thermal energy. In this work, we realized modi¯cations in the MHD two-dimensional model of T. Ogino (1986) in order to include inclination to the magnetic dipolar axis and studied the formation of the magnetosphere for di®erent conditions of Interplanetary Magnetic Field (IMF) and dipole tilts. Additionally to this change, the box simulation was increased and the boundary conditions were changed. In order to assure the modi¯cations were well implemented, we run the code considering a null IMF and three di®erent values of inclination: 0±, 45± e 90±. The obtained results are in good agreement with the ones presented by Wu (Journal of Geophysical Research, 11.048-11.052, 1984) for the same conditions. We also present results that were obtained with initial conditions considering northward and southward IMF, for the three values of dipole tilt. The time evolution of plasma parameters (current and pressure) at the magnetosphere are presented. |
| Área | FISPLASMA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAP > Adding dipole tilt... |
| Conteúdo da Pasta doc | não têm arquivos |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| Idioma | pt |
| Grupo de Usuários | administrator simone administrator |
| Visibilidade | shown |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ET2RFS |
| Acervo Hospedeiro | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
| 6. Notas | |
| Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark type url versiontype volume |
| 7. Controle da descrição | |
| e-Mail (login) | marciana |
| atualizar | |