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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemarte3.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YCT/GSskb
Repositóriosid.inpe.br/iris@1905/2005/07.25.22.22   (acesso restrito)
Última Atualização2017:12.01.15.52.20 (UTC) marciana
Repositório de Metadadossid.inpe.br/iris@1905/2005/07.25.22.22.16
Última Atualização dos Metadados2018:06.06.04.40.10 (UTC) administrator
Chave SecundáriaINPE-7352-PRE/3242
ISSN0034-4672
Rótulo3071
Chave de CitaçãoYanoTaka:1971:ObInRa
TítuloObservation of the intensity ratio between (5,1)and (9,4)bands of OH emission in the night airglow
ProjetoLUME
Ano1971
Data Secundária20000117
Data de Acesso26 jun. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho360 KiB
2. Contextualização
Autor1 Yano, Kyo
2 Takahashi, Hisao
Grupo1 DGE-INPE-BR
RevistaReport of Ionosphere and Space Research in Japan
Volume25
Número4
Páginas302-317
Histórico (UTC)2014-09-29 15:30:54 :: administrator -> marciana :: 1971
2017-12-01 15:52:20 :: marciana -> administrator :: 1971
2018-06-06 04:40:10 :: administrator -> marciana :: 1971
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-ChaveAERONOMIA
EMISSAO DE OXIGENIO
LUMINESCENCIA
FOTOMETRO
ResumoObservations were made of the intensity ratio of (5, 1)to (9, 4)bands of OH emission in the nightglow during a term from November 1968 to October 1969 with an interference filter tilting photometer. The methods of evaluating the ratio from photometer readings are described in some detail. About 245 values of the ratio were obtained on 25 clear nights in the twelve months, scattering around 1.7 with the maximum of 2.1 and the minimum of 1.4. Although some consistency of its monthly variation was found, no regularity such as seasonal variation could be ascertained because observations were obtained through only one year. It was also revealed that on more than half of the observed nights the ratio was roughly constant in the course of night except in twilight conditions, while a nocturnal change from 1.4 up to 2.1 was observed on several occasions. These results are interpreted in terms of the vibrational population of OH molecules in he ground state. It is suggested that the OH molecules in the upper atmosphere could be produced through various kinds of chemical. reactions with different amounts of energy being released, and that there might be a change in the rate of each reaction contributing to the OH formation with a characteristic time of only a few hours duration.
ÁreaCEA
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4. Condições de acesso e uso
Arquivo Alvo7352.pdf
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Grupo de Leitoresadministrator
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Visibilidadeshown
Política de Arquivamentodenypublisher denyfinaldraft
Permissão de Leituradeny from all and allow from 150.163
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5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citando
DivulgaçãoWEBSCI
Acervo Hospedeirosid.inpe.br/banon/2001/04.03.15.36
6. Notas
Campos Vaziosaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Controle da descrição
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