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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3RFK6JL
Repositóriosid.inpe.br/mtc-m21c/2018/07.18.15.21
Última Atualização2021:03.08.19.51.29 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2018/07.18.15.21.06
Última Atualização dos Metadados2021:03.08.19.51.30 (UTC) simone
Chave SecundáriaINPE--PRE/
Chave de CitaçãoBisoiSaJaYaAwSr:2018:FiHiTi
TítuloEvidence of a distant decimetric spike source connected to the main electron acceleration site: first high time cadence gmrt observations
Ano2018
Data de Acesso01 maio 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho61 KiB
2. Contextualização
Autor1 Bisoi, Susanta Kumar
2 Sawant, Hanumant Shankar
3 Janardhan, Padmanabhan
4 Yan, Yihua
5 Awasthi, Kumar
6 Srivastava, Shweta
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHBU
Grupo1
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 National Astronomical Observatories Of China (NAOC)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Physical Research Laboratory
4 National Astronomical Observatories Of China (NAOC)
5 University of Science and Technology of China
6 University of Science and Technology of China, H
Endereço de e-Mail do Autor1 susanta@nao.cas.cn
2 sawant@das.inpe.br
3 janardhan.padmanabhan@gmail.com
4 yyh@nao.cas.cn
5 arun.awasthi.87@gmail.com
6 srivashweta@gmail.com
Nome do EventoCospar Scientific Assembly, 42
Localização do EventoPasadena, California
Data14-22 July
Histórico (UTC)2018-07-18 15:22:47 :: simone -> administrator :: 2018
2019-01-04 16:57:07 :: administrator -> simone :: 2018
2019-01-07 13:00:57 :: simone -> administrator :: 2018
2019-01-14 17:06:31 :: administrator -> simone :: 2018
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoWe present a study of decimetric radio activity, associated with two (GOES C1.4 and M1.0 class) flares and a coronal mass ejection (CME) of 20 June 2015, using the first high time cadence (0.5s) 610 MHz observations of the Giant Meterwave Radio Telescope (GMRT). The GMRT images show strong radio sources during the M1.0 flare and CME, which are located near the flaring site, while, in contrary, a strong spike radio source during the C1.4 flare, with no corresponding coronal or magnetic features, are rather located about 500 arcsec away from the flare site in soft X-rays. Although weak radio burst sources are located near the flaring site, during the C1.4 flare maximum, associated with the spike radio source, which show a good temporal correspondence with a metric typeIII burst identified by the Solar Broadband Radio Spectrometer at Yunnan Astronomical Observatory. A multi-wavelength analysis, in combination with potential field source surface extrapolation, has been carried out to investigate the genesis of non-thermal radio emitting electrons, which revealed that the distant spike radio source, noticed during the C1.4 flare, is actually connected to the main electron acceleration sites and is generated by a plasma emission instead of a loss cone maser instability.
ÁreaCEA
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34R/3RFK6JL
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34R/3RFK6JL
Idiomaen
Arquivo Alvobisoi_evidence.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
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