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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositóriosid.inpe.br/mtc-m17@80/2007/12.17.13.39
Repositório de Metadadossid.inpe.br/mtc-m17@80/2007/12.17.13.39.15
Última Atualização dos Metadados2018:06.05.03.36.35 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoDalLagoInheViei:2007:ObCoMa
TítuloObservations of coronal mass ejections beyond 32 solar radii using STEREO/SECCHI
Ano2007
Data de Acesso19 maio 2024
Tipo SecundárioPRE CN
2. Contextualização
Autor1 Dal Lago, Alisson
2 Inhester, B.
3 Vieira, L. E. A.
Grupo1 DGE-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Max-Planck-Institute for Solar System Research - MPS
3 Max-Planck-Institute for Solar System Research - MPS
Nome do EventoEncontro Brasileiro de Física dos Plasmas, 9.
Localização do EventoSão Pedro, SP
Data25-28 Nov.
Histórico (UTC)2007-12-17 13:39:15 :: simone -> administrator ::
2012-10-24 00:13:20 :: administrator -> simone ::
2013-02-20 15:20:14 :: simone -> administrator :: 2007
2018-06-05 03:36:35 :: administrator -> marciana :: 2007
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoThe Solar TErrestrial RElations Observatory - STEREO was launched on October 25th, 2006 and is composed of two nearly identical spacecrafts, one ahead of Earth in its orbit, the other trailing behind - to provide the ¯rst- ever stereoscopic measurements to study the Sun and the nature of its coronal mass ejections, or CMEs. Each spacecraft has, among others, an instrument package called Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI), which is composed by 4 sets of instruments: SECCHI EUVI: Extreme UltraViolet Imager; SECCHI COR1: Inner Coronagraph; SECCHI COR2: Outer Coronagraph; SECCHI HI: Heliospheric Imager. These instruments will study the evolution of CME's from birth at the Sun's surface through the corona and interplanetary medium to its eventual impact at Earth. Since 1996, the Large Angle and Spectrometric Coronagraph (LASCO), aborde the Solar and Heliospheric Observatory (SOHO), is able to observe the solar corona from 1.1 to 32 solar radii (LASCO C1, C2 and C3 ¯eld of view). This observation capability has improved substantialy since STEREO SECCHI package is able to observe from 1.4 solar radii up to 1 AU (earth orbit). In this work, we show some preliminary observations and measurements of CMEs from 1.4 to beyond 32 solar radii, usind observations from the SECCHI package. Since the SOHO is still in operation, we can perform combined measurements from both SECCHI and LASCO for a few CMEs occurred since STEREO started its observations.
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4. Condições de acesso e uso
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Grupo de Usuáriosadministrator
simone
administrator
Visibilidadeshown
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Acervo Hospedeirolcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
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