| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | mtc-m16b.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 6qtX3pFwXQZGivnK2Y/UnpDL |
| Repositório | sid.inpe.br/mtc-m17@80/2008/06.05.18.37 (acesso restrito) |
| Última Atualização | 2008:06.05.18.37.20 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m17@80/2008/06.05.18.37.21 |
| Última Atualização dos Metadados | 2018:06.05.03.30.49 (UTC) administrator |
| Chave Secundária | INPE--PRE/ |
| DOI | 10.1007/s11207-008-9145-4 |
| ISSN | 0038-0938 1573-093X |
| Chave de Citação | Kane:2008:SiDiTh |
| Título | Similarities and Dissimilarities between the Variations of CME and Other Solar Parameters at Different Heliographic Latitudes and Time Scales  |
| Ano | 2008 |
| Mês | Mar. |
| Data de Acesso | 07 maio 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 674 KiB |
| 2. Contextualização | |
| Autor | Kane, Rajaram Purushotam |
| Grupo | DGE-CEA-INPE-MCT-BR |
| Afiliação | Instituto Nacional de Pesquisas Espaciais (INPE) |
| Revista | Solar Physics |
| Volume | 248 |
| Número | 1 |
| Páginas | 177-190 |
| Histórico (UTC) | 2008-06-05 18:37:21 :: simone -> administrator :: 2010-05-11 02:44:00 :: administrator -> simone :: 2011-05-27 18:38:07 :: simone -> administrator :: 2012-07-13 22:32:40 :: administrator -> simone :: 2008 2013-02-20 15:20:19 :: simone -> administrator :: 2008 2018-06-05 03:30:49 :: administrator -> marciana :: 2008 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Tipo do Conteúdo | External Contribution |
| Palavras-Chave | CORONAL MASS EJECTIONS GROUP SUNSPOT NUMBERS ACTIVITY RECONSTRUCTION CYCLE VARIATION INDEXES FLUX |
| Resumo | From the LASCO CME (Coronal Mass Ejection) catalog, the occurrence frequencies of all CMEs (all strong and weak CMEs, irrespective of their widths) were calculated for 3-month intervals and their 12-month running means determined for cycle 23 (1996-2007) and were compared with those of other solar parameters. The annual values of all-CME frequency were very well correlated (+ 0.97) with sunspot numbers, but several other parameters also had similarly high correlations. Comparisons of 12-month running means indicated that the sunspot numbers were very well correlated with solar electromagnetic radiations (Lyman-alpha, 2800-MHz flux, coronal green line index, solar flare indices, and X-ray background); but for corpuscular radiations [proton fluxes, solar energetic particles (SEP), CMEs, interplanetary CMEs (ICMEs), and stream interaction regions (SIR)] and solar open magnetic fields, the correlations were lower. A notable feature was the appearance of two peaks during 2000-2002, and those double peaks in different parameters matched approximately except for proton fluxes and SEP and SIR frequencies. When hemispheric intensities were considered, north-south asymmetries appeared, more in some parameters than in others. When intensities in smaller latitude belts (10 degrees) were compared, sunspot group numbers (SGN) were found to be confined mostly to latitudes within +/- 30 degrees of the solar equator, showing two peaks in all latitude belts, and during the course of the 11-year cycle, the double peaks shifted from middle to equatorial solar latitudes, just as seen in the Maunder butterfly diagrams. In contrast, CME frequency was comparable at all latitude belts (including high, near-polar latitudes), having more than two peaks in almost all latitude belts, and the peaks were almost simultaneous in all latitude belts. Thus, the matching of SGN peaks with those of CME peaks was poor. Incidentally, the CME frequency data for all events (all widths) after 2003 are not comparable to earlier data, owing to inclusion of very weak (narrow) CMEs in later years. The frequencies are comparable with earlier data only for widths exceeding about 70(degrees). |
| Área | CEA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Similarities and Dissimilarities... |
| 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 | |
| Idioma | en |
| Arquivo Alvo | similarities.pdf |
| Grupo de Usuários | administrator simone |
| Visibilidade | shown |
| Política de Arquivamento | denypublisher denyfinaldraft12 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
| Divulgação | WEBSCI; PORTALCAPES. |
| Acervo Hospedeiro | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Controle da descrição | |
| e-Mail (login) | marciana |
| atualizar | |