1. Identificação | |
Tipo de Referência | Artigo em Evento (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/3QTFHJ8 |
Repositório | sid.inpe.br/mtc-m21c/2018/04.16.13.22 |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2018/04.16.13.22.37 |
Última Atualização dos Metadados | 2020:12.07.21.11.28 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
Chave de Citação | CintraFernRosaSodr:2018:StStTy |
Título | Studying the stochasticity of type I solar storms with gradient spectra |
Ano | 2018 |
Data de Acesso | 09 maio 2024 |
Tipo Secundário | PRE CI |
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2. Contextualização | |
Autor | 1 Cintra, M. A. U. 2 Fernandes, F. C. R. 3 Rosa, Reinaldo Roberto 4 Sodré, Z. A. L. |
Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JJ5D |
Grupo | 1 2 3 LABAC-COCTE-INPE-MCTIC-GOV-BR |
Afiliação | 1 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 Autor | 1 2 3 reinaldo.rosa@inpe.br |
Nome do Evento | Latin American Conference on Space Geophysics, 11 (COLAGE) |
Localização do Evento | Buenos Aires, Argentina |
Data | 16-20 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 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Resumo | It 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. |
Área | COMP |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAC > Studying the stochasticity... |
Conteúdo da Pasta doc | não têm arquivos |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Grupo de Usuários | simone |
Visibilidade | shown |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ESGTTP |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | archivingpolicy 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 |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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