UVIS observations of the FUV OI and CO 4
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B. Hubert; J.C. GΓ©rard; J. Gustin; V.I. Shematovich; D.V. Bisikalo; A.I. Stewart
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Article
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2010
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Elsevier Science
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English
β 577 KB
We analyze FUV spatially-resolved dayglow spectra obtained at 0.37 nm resolution by the UVIS instrument during the Cassini flyby of Venus. We use a least-squares fit method to determine the brightness of the OI emissions at 130.4 and OI 135.6 nm, and of the bands of the CO fourth positive system whi