1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/42JAMPS |
Repositório | sid.inpe.br/mtc-m21c/2020/05.29.11.19 (acesso restrito) |
Última Atualização | 2020:05.29.11.19.32 (UTC) simone |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2020/05.29.11.19.32 |
Última Atualização dos Metadados | 2022:01.04.01.35.10 (UTC) administrator |
DOI | 10.1016/j.asr.2020.03.036 |
ISSN | 0273-1177 1879-1948 |
Chave de Citação | EcherBolzFran:2020:UlObEc |
Título | Statistical analysis of solar wind parameter variation with heliospheric distance: Ulysses observations in the ecliptic plane |
Ano | 2020 |
Mês | June |
Data de Acesso | 01 maio 2024 |
Tipo de Trabalho | journal article |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 2580 KiB |
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2. Contextualização | |
Autor | 1 Echer, Ezequiel 2 Bolzan, Maurício J. A. 3 Franco, Adriane Marques de Souza |
Identificador de Curriculo | 1 8JMKD3MGP5W/3C9JH3D |
Grupo | 1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 2 3 YYY-CGCEA-INPE-MCTIC-GOV-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Universidade Federal de Jataí 3 Instituto Nacional de Pesquisas Espaciais (INPE) |
Endereço de e-Mail do Autor | 1 ezequiel.echer@inpe.br 2 mauricio.bolzam@cnpq.br |
Revista | Advances in Space Research |
Volume | 65 |
Número | 12 |
Páginas | 2846-2856 |
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) | 2020-05-29 11:19:32 :: simone -> administrator :: 2020-05-29 11:19:33 :: administrator -> simone :: 2020 2020-05-29 11:20:05 :: simone -> administrator :: 2020 2022-01-04 01:35:10 :: administrator -> simone :: 2020 |
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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 | Solar wind turbulence Ulysses spacecraft Kurtosis technique Wavelet analysis |
Resumo | The interplanetary magnetic field magnitude B-o, proton density N-p and solar wind speed V, data from Ulysses spacecraft during its interplanetary cruise interval from Earth to Jupiter, from 18 November 1990 to 31 January 1992, are analyzed in this study. Statistical and wavelet techniques are employed to characterize some properties from the solar wind parameters near the ecliptic plane and their dependence with radial distance. The results from kurtosis analysis showed that the three solar wind parameters (B-o, and N-p and V-sw) presented a decrease of this statistical quantity with the increase of scales, indicating that these variables are intermittent in short time scales. Further, the kurtosis parameter presented an increase in all scales around 2-3 AU distance range that corresponds to a solar wind regime transition. It was noted that the interplanetary medium was dominated by solar transients (interplanetary coronal mass ejections) until the middle of 1991. Afterwards a more stable pattern of corotating interaction regions arose. Furthermore, the probability distribution functions presented a spreading shape due to the occurrence of intermittence. In order to study the temporal variability of the solar wind parameters, the wavelet approach was used. The following major periodicities were found for the three solar wind variables studied: similar to 13, similar to 26, and similar to 83-88 days. It was noted that the similar to 13 day periods presented strong spectral power in the 2 to 4 AU range, where the solar wind was dominated by ICME transients. On the other hand, the 26 day period shows higher spectral power for distances higher than 4 AU, where the interplanetary space is more dominated by CIRs. Thus, it was found in this paper a significant dependence of solar wind parameters on radial heliocentric distance which can be accounted by the dynamical evolution of solar wind structures with distance. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Statistical analysis of... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > YYY-PCI-CGCEA > Statistical analysis of... |
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 | echer_statistical.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 |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/4467GD8 |
Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 4 sid.inpe.br/bibdigital/2021/02.11.01.58 3 sid.inpe.br/bibdigital/2013/10.01.22.11 2 |
Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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