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pubmed-article:17750345pubmed:issue3924lld:pubmed
pubmed-article:17750345pubmed:dateCreated2010-6-7lld:pubmed
pubmed-article:17750345pubmed:abstractTextThe predicted intensities of the ionized carbon dioxide (CO(2)+) emission feature at 2890 angstroms and the Fox-Duffendack-Barker bands are 5.2 and 19.9 kilorayleighs, respectively, for a vertical column. Direct photoionization of carbon dioxide by solar radiation contributes 3.5 and 4.1 kilorayleighs, respectively, and fluorescent scattering by C0(2)+, 1.6 and 15.3 kilorayleighs, respectively. Photoelectron impacts are less important.lld:pubmed
pubmed-article:17750345pubmed:languageenglld:pubmed
pubmed-article:17750345pubmed:journalhttp://linkedlifedata.com/r...lld:pubmed
pubmed-article:17750345pubmed:statusPubMed-not-MEDLINElld:pubmed
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pubmed-article:17750345pubmed:issn0036-8075lld:pubmed
pubmed-article:17750345pubmed:authorpubmed-author:DalgarnoAAlld:pubmed
pubmed-article:17750345pubmed:authorpubmed-author:StewartA IAIlld:pubmed
pubmed-article:17750345pubmed:authorpubmed-author:DeggesT CTClld:pubmed
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pubmed-article:17750345pubmed:volume167lld:pubmed
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pubmed-article:17750345pubmed:pagination1490-1lld:pubmed
pubmed-article:17750345pubmed:year1970lld:pubmed
pubmed-article:17750345pubmed:articleTitleMariner 6: origin of Mars ionized carbon dioxide ultraviolet spectrum.lld:pubmed
pubmed-article:17750345pubmed:publicationTypeJournal Articlelld:pubmed