| 1. Identificação | ||||
| Tipo de Referência | Artigo em Revista Científica (Journal Article) | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identificador | 8JMKD3MGP3W34T/459H5A8 | |||
| Repositório | sid.inpe.br/mtc-m21d/2021/08.16.19.04 (acesso restrito) | |||
| Última Atualização | 2021:08.16.19.04.20 (UTC) simone | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21d/2021/08.16.19.04.20 | |||
| Última Atualização dos Metadados | 2022:04.03.19.23.59 (UTC) administrator | |||
| DOI | 10.1016/j.asr.2021.04.034 | |||
| ISSN | 0273-1177 1879-1948 | |||
| Chave de Citação | TiradoBuenoMendMend:2021:BaCoDe | |||
| Título | Barometric coefficient dependence on the geomagnetic cutoff rigidity of neutron monitors  | |||
| Ano | 2021 | |||
| Mês | Sept. | |||
| Data de Acesso | 13 maio 2024 | |||
| Tipo de Trabalho | journal article | |||
| Tipo Secundário | PRE PI | |||
| Número de Arquivos | 1 | |||
| Tamanho | 1026 KiB | |||
| 2. Contextualização | ||||
| Autor | 1 Tirado Bueno, Eduardo 2 Mendoza Torres, J. Eduardo 3 Mendonça, Rafael Rodrigues Souza de | |||
| Grupo | 1 2 3 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 National Institute of Astrophysics Optics and Electronics 2 National Institute of Astrophysics Optics and Electronics 3 Instituto Nacional de Pesquisas Espaciais (INPE) | |||
| Revista | Advances in Space Research | |||
| Volume | 68 | |||
| Número | 6 | |||
| Páginas | 2631-2642 | |||
| Nota Secundária | B1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I | |||
| Histórico (UTC) | 2021-08-16 19:04:20 :: simone -> administrator :: 2021-08-16 19:04:21 :: administrator -> simone :: 2021 2021-08-16 19:06:04 :: simone -> administrator :: 2021 2022-04-03 19:23:59 :: administrator -> simone :: 2021 | |||
| 3. Conteúdo e estrutura | ||||
| É a matriz ou uma cópia? | é a matriz | |||
| Estágio do Conteúdo | concluido | |||
| Transferível | 1 | |||
| Tipo do Conteúdo | External Contribution | |||
| Tipo de Versão | publisher | |||
| Palavras-Chave | Cosmic raysBarometric effectGeomagnetic cutoff rigidity | |||
| Resumo | Several studies have been showing that cosmic ray intensity variations observed at the Earth surface can be a useful tool to analyze and predict space weather and climate phenomena. However, before reach the ground level, the cosmic ray particles interact with dif-ferent atmospheric atoms. This results in the generation of different secondary particles that are differently affected by atmospheric effects. For example, data from neutron monitors, which are widely used to study cosmic ray flux changes related to space phenomena, are significantly affected by atmospheric pressure changes. Thus, for a more detailed study of these instruments' data, it is necessary to know very well how works the pressure affects secondary neutrons. In this way, we seek to understand how this effect changes according to the cosmic rays' energy. Thus, in this work, we compare how the barometric coefficient (beta), which quantifies the pressure effect on the cosmic ray intensity, changes with the geomagnetic cutoff rigidity (R-C), which quantifies the minimal rigidity/energy that a primary particle needs to reach a given location in a chosen direction. To do that, we used data recorded between January 2008 to December 2016 by several neutron monitors around the globe with R-C from 0.1 to 8.3 GV. We experimentally obtained beta in two ways: (I) the typical one, which does not explicitly consider isotropic variations unrelated to the pressure effect; and (II) one that considers such variations by using coupling coefficients and a reference neutron monitor station. Like other works, we found that the pressure effect seems to present a logarithmic relation with the cutoff rigidity when we estimate beta through the typical method used. On the other hand, we found that the pressure effect linearly decreases with the cutoff rigidity when considering an adjustment in this typical method to eliminate external isotropic variations. This linear relation appears to not change accordingly to the reference monitor chosen. These results enhance our knowledge of how the pressure effect globally acts on the cosmic ray intensity observed at ground level and, consequently, improves future analysis about global changes in the cosmic ray flux related to space weather phenomena. | |||
| Área | CEA | |||
| Arranjo | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Barometric coefficient dependence... | |||
| Conteúdo da Pasta doc | acessar | |||
| Conteúdo da Pasta source | não têm arquivos | |||
| Conteúdo da Pasta agreement |
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| 4. Condições de acesso e uso | ||||
| Idioma | en | |||
| Arquivo Alvo | tirado_barometric.pdf | |||
| Grupo de Usuários | simone | |||
| Grupo de Leitores | administrator simone | |||
| Visibilidade | shown | |||
| Política de Arquivamento | denypublisher denyfinaldraft24 | |||
| Permissão de Leitura | deny from all and allow from 150.163 | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/46KTFK8 | |||
| Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. | |||
| Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notas | ||||
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||