The 825–1110 Å EUV Spectrum of Venus
✍ Scribed by S.Alan Stern; David C. Slater; G.Randall Gladstone; Erik Wilkenson; Webster C. Cash; James C. Green; Donald M. Hunten; Tobias C. Owen; Larry Paxton
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 201 KB
- Volume
- 122
- Category
- Article
- ISSN
- 0019-1035
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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
Equilibrium population of Fextv levels in coronal conditions was calculated including configurations 3sZ3p, 3s3p ~, 3s23d, 3p 3, 3s3p3d, 3s~4s, 3s24p, 3s24d, 3s~4f Relative populations of selected levels are given in Table VII. Figure 1 shows the dependence of relative intensities of the strongest l