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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3PPT9U5
Repositóriosid.inpe.br/mtc-m21b/2017/10.10.13.08
Última Atualização2017:10.10.13.08.22 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21b/2017/10.10.13.08.22
Última Atualização dos Metadados2022:03.08.17.26.14 (UTC) administrator
DOI10.5194/acp-2017-185
ISSN1680-7367
Chave de CitaçãoCecchiniMWCKAAAABFKMMMMPPPPRW:2017:InPoAp
TítuloIllustration of microphysical processes in Amazonian deep convective clouds in the Gamma phase space: introduction and potential applications
Ano2017
Mêsmarc.
Data de Acesso13 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1954 KiB
2. Contextualização
Autor 1 Cecchini, Micael Amore
 2 Machado, Luiz Augusto Toledo
 3 Wendisch, Manfred
 4 Costa, Anja
 5 Krämer, Martina
 6 Andreae, Meinrat O.
 7 Afchine, Armin
 8 Albrecht, Rachel I.
 9 Artaxo, Paulo
10 Borrmann, Stephan
11 Fütterer, Daniel
12 Klimach, Thomas
13 Mahnke, Christoph
14 Martin, Scot T.
15 Minikin, Andreas
16 Molleker, Sergej
17 Pardo, Lianet Hernández
18 Pöhlker, Christopher
19 Pöhlker, Mira L.
20 Pöschl, Ulrich
21 Rosenfeld, Daniel
22 Weinzierl, Bernadett
Identificador de Curriculo 1
 2 8JMKD3MGP5W/3C9JHMS
Grupo 1 MET-MET-SESPG-INPE-MCTIC-GOV-BR
 2 DIDSA-CGCPT-INPE-MCTIC-GOV-BR
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17 MET-MET-SESPG-INPE-MCTIC-GOV-BR
Afiliação 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Universität Leipzig
 4 Institut für Energie und Klimaforschung (IEK-7)
 5 Institut für Energie und Klimaforschung (IEK-7)
 6 Max Planck Institute for Chemistry
 7 Institut für Energie und Klimaforschung (IEK-7)
 8 Universidade de São Paulo (USP)
 9 Universidade de São Paulo (USP)
10 Max Planck Institute for Chemistry
11 Deutsches Zentrum für Luft- und Raumfahrt (DLR)
12 Max Planck Institute for Chemistry
13 Max Planck Institute for Chemistry
14 Harvard University
15 Deutsches Zentrum für Luft- und Raumfahrt (DLR)
16 Johannes Gutenberg-Universität
17 Instituto Nacional de Pesquisas Espaciais (INPE)
18 Max Planck Institute for Chemistry
19 Max Planck Institute for Chemistry
20 Max Planck Institute for Chemistry
21 The Hebrew University of Jerusalem
22 Deutsches Zentrum für Luft- und Raumfahrt (DLR)
Endereço de e-Mail do Autor 1 micael.cecchini@gmail.com
 2 luiz.machado@inpe.br
RevistaAtmospheric Chemistry and Physics Discussion
Volume185
Páginas1-49
Nota SecundáriaC_ASTRONOMIA_/_FÍSICA
Histórico (UTC)2017-10-10 13:08:22 :: simone -> administrator ::
2017-10-10 13:08:23 :: administrator -> simone :: 2017
2017-10-10 13:11:11 :: simone -> administrator :: 2017
2017-10-14 02:57:14 :: administrator -> simone :: 2017
2017-12-11 18:15:51 :: simone -> administrator :: 2017
2022-03-08 17:26:14 :: administrator -> simone :: 2017
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
ResumoThe behavior of tropical clouds remains a major open scientific question, given that the associated physics is not well represented by models. One challenge is to realistically reproduce cloud droplet size distributions (DSD) and their evolution over time and space. Many applications, not limited to models, use the Gamma function to represent DSDs. However, there is almost no study dedicated to understanding the phase space of this function, which is given by the three parameters that define the DSD intercept, shape, and curvature. Gamma phase space may provide a common framework for parameterizations and inter-comparisons. Here, we introduce the phase-space approach and its characteristics, focusing on warm-phase microphysical cloud properties and the transition to the mixed-phase layer. We show that trajectories in this phase space can represent DSD evolution and can be related to growth processes. Condensational and collisional growth may be interpreted as pseudo-forces that induce displacements in opposite directions within the phase space. The actually observed movements in the phase space are a result of the combination of such pseudo-forces. Additionally, aerosol effects can be evaluated given their significant impact on DSDs. The DSDs associated with liquid droplets that favor cloud glaciation can be delimited in the phase space, which can help models to adequately predict the transition to the mixed phase. We also consider possible ways to constrain the DSD in two-moment bulk microphysics schemes, where the relative dispersion parameter of the DSD can play a significant role. Overall, the Gamma phase-space approach can be an invaluable tool for studying cloud microphysical evolution and can be readily applied in many scenarios that rely on Gamma DSDs.
ÁreaMET
Arranjo 1urlib.net > BDMCI > MET > Illustration of microphysical...
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34P/3PPT9U5
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34P/3PPT9U5
Idiomaen
Arquivo Alvocecchini_illustration.pdf
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5. Fontes relacionadas
Vinculação8JMKD3MGP3W34P/3NKDGFS
Repositório Espelhosid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Unidades Imediatamente Superiores8JMKD3MGPCW/3F35TRS
8JMKD3MGPCW/43SRC6S
Lista de Itens Citandosid.inpe.br/bibdigital/2021/01.03.02.10 2
DivulgaçãoWEBSCI; PORTALCAPES; MGA.
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarytype url
7. Controle da descrição
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