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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositóriosid.inpe.br/mtc-m17@80/2007/11.21.03.50
Repositório de Metadadossid.inpe.br/mtc-m17@80/2007/11.21.03.50.39
Última Atualização dos Metadados2018:06.05.03.35.17 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoBertagnolliSchPosPinFer:2007:2020
TítuloWavelets in the Study of the Secondary Effects of the Antarctic Ozone hole at the Southern Space Observatory: 2003 – 2005
Ano2007
Data de Acesso18 maio 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Bertagnolli, Carolina
2 Schuch, Nelson Jorge
3 Possani, Germano
4 Pinheiro, Damaris Kirsch
5 Ferreira, Nelson Jesus
Grupo1 RSU-INPE-MCT-BR
2 RSU-INPE-MCT-BR
3 RSU-INPE-MCT-BR
4
5 CPT-INPE-MCT-BR
Afiliação1 Southern Regional Space Research Center – CRS/INPE – MCT, Santa Maria, RS, Brazil
2 Southern Regional Space Research Center – CRS/INPE – MCT, Santa Maria, RS, Brazil
3 Southern Regional Space Research Center – CRS/INPE – MCT, Santa Maria, RS, Brazil
4 Space Science Laboratory of Santa Maria – LACESM/CT – UFSM, Santa Maria, Brazil
5 National Institute for Space Research – CPTEC/INPE – MCT, São José dos Campos, SP, Brazil
Nome do EventoIUGG General Assembly, 24.
Localização do EventoPerugia, Italy
Data2-13 July
Título do LivroProceedings
Tipo TerciárioPoster Session
Histórico (UTC)2007-11-21 03:57:16 :: seeger05 -> administrator ::
2018-06-05 03:35:17 :: administrator -> seeger05 :: 2007
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveWavelets
Ozone
Antarctic Ozone Hole
Secondary Effects – Química da Atmosfera
ResumoThe secondary effects of the Antarctic ozone hole have been a local perturbation in the ozone content to low latitudes for several years. Wavelet transform is applied for characterization of this phenomenon at Southern Space Observatory, SSO/CRS/INPE MCT (29.4ºS, 53.8ºW) at São Martinho da Serra, Brazil, during the years 2003, 2004 and 2005. The total ozone column data from Spectrophotometer Brewer MKIII#167 and TOMS are used. The spectrophotometer measures total ozone column on the wavelengths: 306.3, 310.1, 313.5, 316.8 and 320.0 nm, while TOMS measures on: 317.5 and 331.2 nm. The effect occurs between the Julian days 200 and 300, period of ozone maximum value at Southern Space Observatory. The years 2003, 2004 and 2005 presents 2, 3 and 1 event of secondary effects of the Antarctic ozone hole respectively. The wavelets continuous spectrums are analyzed for the three years separately and show the influence of the secondary effects to low latitudes with duration about 2.3 days for all years.
ÁreaCEA
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4. Condições de acesso e uso
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Visibilidadeshown
Permissão de Leituradeny from all and allow from 150.163
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/3EUPEJL
Acervo Hospedeirolcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark type url versiontype volume
7. Controle da descrição
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