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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP8W/35SNTG5
Repositóriosid.inpe.br/mtc-m18@80/2009/08.21.15.41
Repositório de Metadadossid.inpe.br/mtc-m18@80/2009/08.21.15.41.57
Última Atualização dos Metadados2020:04.28.17.49.00 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoDalLagoInheViei:2009:Ja20CM
TítuloThe January 2007 CME observed with stereo/secchi and soho/lasco and its arrival at venus
Ano2009
Data de Acesso26 jun. 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Dal Lago, Alisson
2 Inhester, Bernd
3 Vieira, Luis Eduardo Antunes
Grupo1 DGE-CEA-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Max-Planck-Institute for Solar System Research
3 Max-Planck-Institute for Solar System Research
Nome do EventoIaga, 2009.
Localização do EventoSopron, Hungary
Data23-30 Aug.
Título do LivroProceedings
Histórico (UTC)2009-08-21 15:41:57 :: simone -> administrator ::
2020-04-28 17:49:00 :: administrator -> simone :: 2009
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveCME
SOHO
STEREO
Venus
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. Its objective is 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 are able to study the evolution of CMEs from birth at the Suns surface through the corona and interplanetary medium. Since 1996, the Large Angle and Spectrometric Coronagraph (LASCO), abord 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 field 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 study the evolution of a CMEs occurred on January 8th 2007 from 1.4 to beyond 32 solar radii, usind observations from the SECCHI package. Since SOHO is still in operation, and since STEREO was very close proximity of the earth during this event, we were able to compare measurements from both SECCHI and LASCO instruments for this same CME. We show estimates of the CME travel time to Venus using distinct approaches and compare with in situ observations.
ÁreaCEA
ArranjoThe January 2007...
Conteúdo da Pasta docnão têm arquivos
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4. Condições de acesso e uso
Idiomaen
Grupo de Usuáriossimone
administrator
Visibilidadeshown
Permissão de Leituraallow from all
5. Fontes relacionadas
Repositório Espelhosid.inpe.br/mtc-m18@80/2008/03.17.15.17.24
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Acervo Hospedeirosid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format isbn issn label lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup 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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