| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | mtc-m16.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 6qtX3pFwXQZ3r59YDa/H2krt |
| Repositório | sid.inpe.br/iris@1916/2005/08.01.14.25 (acesso restrito) |
| Última Atualização | 2005:08.01.03.00.00 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/iris@1916/2005/08.01.14.25.40 |
| Última Atualização dos Metadados | 2018:06.05.01.16.06 (UTC) administrator |
| Chave Secundária | INPE-12915-PRE/8197 |
| ISSN | 0038-0938 1573-093X |
| Chave de Citação | SilvaLaCaKaCoLeRo:2005:DiCoSp |
| Título | Diffuse component spectra of solar active regions at submillimeter wavelengths  |
| Projeto | Radiofísica / CRAAM: Centro de radioastronomia e astrofísica |
| Ano | 2005 |
| Mês | Apr. |
| Data de Acesso | 26 jun. 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 362 KiB |
| 2. Contextualização | |
| Autor | 1 Silva, Adriana V. R. 2 Lagana, Tatiana F. 3 Castro, C. Guillermo Gimenez de 4 Kaufmann, Pierre 5 Costa, Joaquim Eduardo Rezende 6 Levato, Hugo 7 Rovira, Marta |
| Identificador de Curriculo | 1 2 3 4 5 8JMKD3MGP5W/3C9JHF8 |
| Grupo | 1 2 3 4 5 DAS-INPE-MCT-BR |
| Afiliação | 1 Universidade Presbiteriana Mackenzie (CRAAM) 2 Universidade Presbiteriana Mackenzie (CRAAM) 3 Universidade Presbiteriana Mackenzie (CRAAM) 4 Universidade Presbiteriana Mackenzie (CRAAM) 5 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS) 6 Complejo Astronómico el Leoncito 7 Instituto de Astronomia y Fisica del Espacio |
| Revista | Solar Physics |
| Volume | 227 |
| Número | 2 |
| Páginas | 265-281 |
| Histórico (UTC) | 2005-08-18 11:11:14 :: sergio -> administrator :: 2006-09-28 22:30:00 :: administrator -> sergio :: 2008-01-07 12:52:53 :: sergio -> marciana :: 2008-04-02 17:17:55 :: marciana -> administrator :: 2008-06-10 22:39:33 :: administrator -> marciana :: 2011-05-21 03:10:15 :: marciana -> administrator :: 2018-06-05 01:16:06 :: administrator -> marciana :: 2005 |
| 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 | ASTROPHYSICS Solar active regions Slowly varying component Radio emission Millimeter wavelengths Sun MM Microns ASTROFÍSICA Regiões solares ativas Emissão de raios Sol |
| Resumo | Solar maps at 212 and 405 GHz obtained by the Solar Submillimetric Telescope (SST) show regions of enhanced brightness temperature, which coincide with the location of active regions. A statistical study of the radio emission from these active regions was performed for the first time at such high frequencies during 23 days on June and July 2002, when the atmospheric opacity was low. The brightest regions on the maps were chosen for this study, where the brightness excess observed varies from 3 to 20% above quiet Sun levels (i.e., 200-1000 K) at both wavelengths. Sizes of the regions of enhanced emission calculated at half the maximum value were estimated to be between 2' and 7'. These sizes agree with observed sizes of active regions at other wavelengths such as H alpha and ultraviolet. An important result is that the flux density spectra of all sources increase toward submillimeter frequencies, yielding flux density spectral index with an average value of 2.0. The flux density of the active region sources were complemented with that from maps at 17 and 34 GHz from the Nobeyama Radio Heliograph. The resulting spectra at all four frequencies were fit considering the flux density to be due to thermal bremsstrahlung from the active region. In the calculations, the source radius was assumed to be the mean of the measured values at 212 and 405 K. The effective temperatures of the radio emitting source, assumed homogeneous, obtained from this fit were 0.6-2.9 x 10(4) K, for source diameters of 2'-7'. |
| Área | CEA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Diffuse component spectra... |
| 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 | diffuse component.pdf |
| Grupo de Usuários | administrator marciana sergio |
| Visibilidade | shown |
| Detentor da Cópia | SID/SCD |
| Política de Arquivamento | denypublisher denyfinaldraft12 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETR8EH |
| Divulgação | WEBSCI; PORTALCAPES. |
| Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Controle da descrição | |
| e-Mail (login) | marciana |
| atualizar | |