| 1. Identificação | |
| Tipo de Referência | Artigo em Evento (Conference Proceedings) |
| Site | mtc-m16.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 6qtX3pFwXQZsFDuKxG/EJrVg |
| Repositório | sid.inpe.br/marciana/2005/01.10.11.39 |
| Última Atualização | 2021:02.23.14.55.43 (UTC) simone |
| Repositório de Metadados | sid.inpe.br/marciana/2005/01.10.11.39.18 |
| Última Atualização dos Metadados | 2021:02.23.14.55.43 (UTC) simone |
| Chave Secundária | INPE--PRE/ |
| Rótulo | self-archiving-INPE-MCTIC-GOV-BR |
| Chave de Citação | GusevTaJaPuScSp:2004:NuMoAn |
| Título | Numerical modeling of the antiproton radiation belt accouting radial diffusion of external interstellar and internal albedo antiprotons and inelastic scattering losses  |
| Ano | 2004 |
| Data de Acesso | 26 dez. 2024 |
| Tipo Secundário | PRE CI |
| Número de Arquivos | 1 |
| Tamanho | 69 KiB |
| 2. Contextualização | |
| Autor | 1 Gusev, Anatoly Alexandrovitch 2 Talavera, Kenny Choque 3 Jayanthi, Udaya Bhaskaram 4 Pugacheva, G. I. 5 Schuch, Nelson Jorge 6 Spjeldvik, W. N. |
| Grupo | 1 DAS-INPE-MCT-BR 2 RSU-INPE-MCT-BR |
| Nome do Evento | Scientific Assembly of COSPAR, (37Th). |
| Localização do Evento | Paris, France |
| Data | 18-25 july |
| Editora (Publisher) | INPE |
| Título do Livro | Anais |
| Histórico (UTC) | 2005-01-10 13:39:20 :: jefferson -> administrator :: 2018-06-05 01:21:25 :: administrator -> marciana :: 2004 2019-03-25 18:08:23 :: marciana -> simone :: 2004 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Resumo | The possible existence of noticeable fluxes of antiprotons in the Earth magnetosphere is considered in this presentation on the base of numerical solution of diffusion equation by FDM (Finite Difference Method) method. The antiprotons geomagnetically confined in the inner magnetosphere at L-shells below L=7 are both the interstellar origin and locally generated antiprotons, i.e. the products of nuclear reactions of the high energy primary cosmic rays (CR) with constituents of the terrestrial atmosphere. The interstellar antiprotons penetrating into the Earth's magnetosphere are themselves secondary in origin, i.e. they are born in nuclear reactions of the same CR passing through 5-7 g/cm^2 of interstellar matter. Until now there was not found some special source of the primary antiprotons. The magnetospheric locally generated antiprotons are born at a pass length of dozens g/cm^2 matter in the residual Earth atmosphere, then, they are confined by the geomagnetic field and accumulated in the magnetosphere. One could expect that their fluxes significantly overcome the interstellar antiproton fluxes. However, just after the birth they undergone to several loss processes such as ionization losses, nuclear reactions and annihilation on the ambient atoms and a diffusion into and out of magnetosphere that makes it is difficult to predict which fluxes will be greater. These processes are included into diffusion theory and solution of the diffusion equation describes the trapped antiproton flux in magnetosphere accounting all above mentioned losses. We present the results of numerical simulation of diffusion equation solution for magnetospheric antiproton fluxes in the energy range from 10 MeV to several GeV originated from both sources: the locally produced and interstellar fluxes which diffused and directly penetrated into magnetosphere from the Earth vicinity. The estimates made show the space distribution of trapped antiprotons and a significant (up to two orders of magnitude) excess of magnetospheric antiproton fluxes over those formed in the interstellar media at energies < 1 to 2 GeV at determined L-shells. |
| Área | CEA |
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Numerical modeling of... |
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Numerical modeling of... |
| Conteúdo da Pasta doc | acessar |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| URL dos dados | http://urlib.net/ibi/6qtX3pFwXQZsFDuKxG/EJrVg |
| URL dos dados zipados | http://urlib.net/zip/6qtX3pFwXQZsFDuKxG/EJrVg |
| Idioma | en |
| Arquivo Alvo | gusev_numerical.pdf |
| Grupo de Usuários | administrator jefferson simone |
| Grupo de Leitores | administrator simone |
| Visibilidade | shown |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETR8EH 8JMKD3MGPCW/3EUFCFP |
| Lista de Itens Citando | sid.inpe.br/bibdigital/2013/10.04.21.53 5 sid.inpe.br/bibdigital/2013/10.01.00.07 1 |
| Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notas | |
| Campos Vazios | affiliation archivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn keywords lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume |
| 7. Controle da descrição | |
| e-Mail (login) | simone |
| atualizar | |