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dc.contributor.advisorBashkin, Stanleyen_US
dc.contributor.authorLeu, Lina, 1962-
dc.creatorLeu, Lina, 1962-en_US
dc.date.accessioned2013-04-03T13:13:20Z
dc.date.available2013-04-03T13:13:20Z
dc.date.issued1992en_US
dc.identifier.urihttp://hdl.handle.net/10150/278112
dc.description.abstractTargets of CO₂ in a differentially-pumped chamber at a pressure of 40 mTorr were bombarded by particles of H₃⁺ at energy of 1 MeV. The optical spectrum created in the collisions was analyzed with a 1-meter, air Czerny-Turner spectrometer. The spectrum excited in the collisions is dominated by molecular bands in the wavelength range from 300 nm to 900 nm. However, one also sees weak atomic lines from C I, C II, O I and O II. The excitation process gives rise to relatively weak atomic spectra in the visible region compared to similar studies of O₂. This paper reports on the carbon dioxide spectra and compares the relative intensities and the line widths of various features with similar studies of oxygen.
dc.language.isoen_USen_US
dc.publisherThe University of Arizona.en_US
dc.rightsCopyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author.en_US
dc.subjectPhysics, Atomic.en_US
dc.titleOptical excitation of carbon dioxide by bombardment with ions of tri-atomic hydrogen at an energy of one million electron-voltsen_US
dc.typetexten_US
dc.typeThesis-Reproduction (electronic)en_US
thesis.degree.grantorUniversity of Arizonaen_US
thesis.degree.levelmastersen_US
dc.identifier.proquest1348478en_US
thesis.degree.disciplineGraduate Collegeen_US
thesis.degree.nameM.S.en_US
dc.identifier.bibrecord.b27580192en_US
refterms.dateFOA2018-08-13T16:31:33Z
html.description.abstractTargets of CO₂ in a differentially-pumped chamber at a pressure of 40 mTorr were bombarded by particles of H₃⁺ at energy of 1 MeV. The optical spectrum created in the collisions was analyzed with a 1-meter, air Czerny-Turner spectrometer. The spectrum excited in the collisions is dominated by molecular bands in the wavelength range from 300 nm to 900 nm. However, one also sees weak atomic lines from C I, C II, O I and O II. The excitation process gives rise to relatively weak atomic spectra in the visible region compared to similar studies of O₂. This paper reports on the carbon dioxide spectra and compares the relative intensities and the line widths of various features with similar studies of oxygen.


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