𝔖 Bobbio Scriptorium
✦   LIBER   ✦

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

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


EUV imaging of near-Venus space
✍ A. Yamazaki; I. Yoshikawa; N. Terada; M. Nakamura 📂 Article 📅 2004 🏛 Elsevier Science 🌐 English ⚖ 573 KB
EUV spectroscopy of the Venus dayglow wi
✍ J.-C. Gérard; B. Hubert; J. Gustin; V.I. Shematovich; D. Bisikalo; G.R. Gladston 📂 Article 📅 2011 🏛 Elsevier Science 🌐 English ⚖ 846 KB

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

Theoretical intensities of Fexivin the s
✍ M. Blaha 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 892 KB

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