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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/3QTFHJ8
Repositóriosid.inpe.br/mtc-m21c/2018/04.16.13.22
Repositório de Metadadossid.inpe.br/mtc-m21c/2018/04.16.13.22.37
Última Atualização dos Metadados2020:12.07.21.11.28 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoCintraFernRosaSodr:2018:StStTy
TítuloStudying the stochasticity of type I solar storms with gradient spectra
Ano2018
Data de Acesso09 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Cintra, M. A. U.
2 Fernandes, F. C. R.
3 Rosa, Reinaldo Roberto
4 Sodré, Z. A. L.
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JJ5D
Grupo1
2
3 LABAC-COCTE-INPE-MCTIC-GOV-BR
Afiliação1 Universidade do Vale do Paraíba (UNIVAP)
2 Universidade do Vale do Paraíba (UNIVAP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidade do Vale do Paraíba (UNIVAP)
Endereço de e-Mail do Autor1
2
3 reinaldo.rosa@inpe.br
Nome do EventoLatin American Conference on Space Geophysics, 11 (COLAGE)
Localização do EventoBuenos Aires, Argentina
Data16-20 abr.
Histórico (UTC)2018-04-16 13:23:00 :: simone -> administrator :: 2018
2018-04-18 05:03:01 :: administrator -> administrator] :: 2018
2018-04-18 05:03:01 :: administrator] -> administrator :: 2018
2020-12-07 21:11:28 :: administrator -> simone :: 2018
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoIt is known that Type I solar emissions are generated by non-thermal electrons accelerated by structural variations in the active regions magnetic configuration. Most of the Type I bursts is recorded as a sequence of individual bursts characterizing the so-called chains of Type I. They, also, could be associated with solar flares. In this case, the flare dissipative energy is added to the energy released by small changes in magnetic distribution, which increases the duration of Type I storms. One of the major challenges to this context is to characterize the underlying stochastic process best suited to describe the noise patterns of Type I storms. We consider that a first step in this direction is to find or discard similarities with type 1/f noises. In this work, by applying the Gradient Pattern Analysis (GPA), we compared the gradient spectra of Type I storms with canonical gradient spectra generated by White, Pink and Red Noises. The data are time series of Type I bursts recorded in metric wavelengths (65 - 865 MHz) by the Compound Astronomical Low cost Low frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) spectrographs. The results accurately indicate that the gradient spectra of Type I solar noise storms captured from CALLISTO are distinct from all type 1/f noises. Thus, considering the results presented here, purely stochastic mechanisms can be discarded as being the major underlying process associated with the plasma dynamics of the phenomenon. In addition, we discuss, from a technical perspective, the advantages of applying GPA over Power Spectral Density (PSD) due to its greater robustness for short series.
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4. Condições de acesso e uso
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Grupo de Usuáriossimone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ESGTTP
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 numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission 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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