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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/3QTFCKS
Repositóriosid.inpe.br/mtc-m21c/2018/04.16.12.22
Repositório de Metadadossid.inpe.br/mtc-m21c/2018/04.16.12.22.54
Última Atualização dos Metadados2020:12.07.21.11.27 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoBerdichevskyRodr:2018:ThInEl
TítuloA thermodynamics interpretation of electron and temperature description in the Sun’s corona
Ano2018
Data de Acesso13 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Berdichevsky, D. B.
2 Rodríguez Gómez, Jenny Marcela
Grupo1
2 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
Afiliação1 Instituto de Física Rosario (IFIR)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 dbberdi@gmail.com
2 jenny.gomez@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 12:23:32 :: simone -> administrator :: 2018
2018-04-18 04:57:43 :: administrator -> administrator] :: 2018
2018-04-18 04:57:43 :: administrator] -> administrator :: 2018
2018-04-18 05:00:02 :: administrator -> administrator] :: 2018
2018-04-18 05:00:02 :: administrator] -> administrator :: 2018
2018-07-04 17:51:12 :: administrator -> simone :: 2018
2018-08-08 11:45:09 :: simone -> administrator :: 2018
2020-12-07 21:11:27 :: 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 reach a thermodynamic interpretation to a model study of electrons density and temperature grounded on the physics of hydro magnetism in global equilibrium. This is the Coronal Density and Temperature (CODET) model of the Sun K-Corona, see bottom sentences. The thermodynamic interpretation finds consistency of the model with a magnetomatter medium that is diamagnetic, in the context of ideal magneto-hydrodynamics. To achieve the result in a quantitative way we propose that this medium possess an underlying structure that was earlier described to explain the adsorption process, i.e. in this case to be a 3-D Langmuir amorphous lattice in thermodynamic equilibrium. In this way constitutive properties of the medium magnetic permeability, the non-dispersive acoustic speed, the expected equilibration time for the 1.1 to 1.3 solar radius region are here discussed, which are determined quantitatively for a portion of the quiescent corona in a near solar minimum that extends for most of years 2008 and almost all 2009. (The CODET model uses as input photosphere magnetic field, this magnetic field is extrapolated through the solar atmosphere from Potential Field Source Surface (PFSS) model. Also, a flux transport model, an emission model and an optimization algorithm are used.).
ÁreaCEA
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4. Condições de acesso e uso
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Grupo de Usuáriossimone
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Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Vinculação8JMKD3MGP3W34P/3NCJQLB
Repositório Espelhourlib.net/www/2011/03.29.20.55
Unidades Imediatamente Superiores8JMKD3MGPCW/3F2NE4L
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 nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarytype type url versiontype volume
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