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
Cassini-UVIS observation of dayglow FUV emissions of carbon in the thermosphere of Venus
✍ Scribed by B. Hubert; J.-C. Gérard; J. Gustin; D.V. Bisikalo; V.I. Shematovich; G.R. Gladstone
- Book ID
- 116535922
- Publisher
- Elsevier Science
- Year
- 2012
- Tongue
- English
- Weight
- 647 KB
- Volume
- 220
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
We analyze EUV spatially-resolved dayglow spectra obtained at 0.37 nm resolution by the UVIS instrument during the Cassini flyby of Venus on 24 June 1999, a period of high solar activity level. Emissions from OI, OII, NI, CI and CII and CO have been identified and their disc average intensity has be
Ro-vibrational band head emissions from highly rotationally-excited NO + (v; J ) (J ¿90) have been observed for quiescent and aurorally disturbed conditions at tangent altitudes between approximately 100 and 215 km in the terrestrial thermosphere. The formation of these band heads in NO + requires v