| 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 | QABCDSTQQW/46AC7UB | |||
| Repositório | urlib.net/www/2022/02.03.21.42 (acesso restrito) | |||
| Última Atualização | 2022:02.03.21.42.27 (UTC) simone | |||
| Repositório de Metadados | urlib.net/www/2022/02.03.21.42.27 | |||
| Última Atualização dos Metadados | 2023:01.03.23.29.30 (UTC) simone | |||
| DOI | 10.26464/epp2022006 | |||
| ISSN | 2096-3955 | |||
| Chave de Citação | FrancoEcheBolzFrae:2022:MaExOb | |||
| Título | Study of fluctuations in the Martian magnetosheath using a kurtosis technique: Mars Express observations  | |||
| Ano | 2022 | |||
| Data de Acesso | 11 maio 2024 | |||
| Tipo de Trabalho | journal article | |||
| Tipo Secundário | PRE PI | |||
| Número de Arquivos | 1 | |||
| Tamanho | 4071 KiB | |||
| 2. Contextualização | ||||
| Autor | 1 Franco, Adriane Marques de Souza 2 Echer, Ezequiel 3 Bolzan, M. J. A. 4 Fraenz, M. | |||
| Identificador de Curriculo | 1 2 8JMKD3MGP5W/3C9JH3D | |||
| Grupo | 1 2 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Universidade Federal de Jatai 4 Mak Planck for Solar System Research | |||
| Endereço de e-Mail do Autor | 1 adriane.marquesds@gmail.com 2 ezequiel.echer@inpe.br | |||
| Revista | Earth and Planetary Physics | |||
| Volume | 6 | |||
| Número | 1 | |||
| Páginas | 28-41 | |||
| Histórico (UTC) | 2022-02-03 21:43:19 :: simone -> administrator :: 2022 2023-01-03 16:46:29 :: administrator -> simone :: 2022 | |||
| 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 | Mars magnetosheath kurtosis ULF waves | |||
| Resumo | Planetary magnetosheaths are characterized by high plasma wave and turbulence activity. The Martian magnetosheath is no exception; both upstream and locally generated plasma waves have been observed in the region between its bow shock and magnetic boundary layer, its induced magnetosphere. This statistical study of wave activity in the Martian magnetosheath is based on 12 years (2005-2016) of observations made during Mars Express (MEX) crossings of the planet's magnetosheath - in particular, data on electron density and temperature data collected by the electron spectrometer (ELS) of the plasma analyzer (ASPERA-3) experiment on board the MEX spacecraft. A kurtosis parameter has been calculated for these plasma parameters. This value indicates intermittent behavior in the data when it is higher than 3 (the value for a normal or Gaussian distribution). The variation of wave activity occurrence has been analyzed in relation to solar cycle, Martian orbit, and distance to the bow shock. Non-Gaussian properties are observed in the magnetosheath of Mars on all analyzed scales, especially in those near the proton gyrofrequency in the upstream region of the Martian magnetosphere. We also report that non-Gaussian behavior is most prominent at the smaller scales (higher frequencies). A significant influence of the solar cycle was also observed; the kurtosis parameter is higher during declining and solar maximum phases, when the presence of disturbed solar wind conditions, caused by large scale solar wind structures, increases. The kurtosis decreases with increasing distance from the bow shock, which indicates that the intermittence level is higher near the bow shock. In the electron temperature data the kurtosis is higher near the perihelion due to the higher incidence of EUV when the planet is closer to the Sun, which causes a more extended exosphere, and consequently increases the wave activity in the magnetosheath and its upstream region. The extended exosphere seems to play a lower effect in the electron density data. | |||
| Área | CEA | |||
| Arranjo | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Study of fluctuations... | |||
| 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 | Study+of+fluctuations+in+the+Martian+magnetosheath+using+a+kurtosis+technique_+Mars+Express+observations.pdf | |||
| Grupo de Usuários | self-uploading-INPE-MCTI-GOV-BR simone | |||
| Grupo de Leitores | administrator simone | |||
| Visibilidade | shown | |||
| Permissão de Leitura | deny from all and allow from 150.163 | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Vinculação | Trabalho não Vinculado à Tese/Dissertação | |||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/46KTFK8 | |||
| Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 5 sid.inpe.br/bibdigital/2022/04.03.17.52 2 | |||
| Divulgação | WEBSCI; SCOPUS. | |||
| Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notas | ||||
| Campos Vazios | alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarytype url | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||