𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The Xray-EUV spectrum of optically thin plasmas

✍ Scribed by B. C. Monsignori Fossi; M. Landini


Publisher
Springer
Year
1994
Tongue
English
Weight
256 KB
Volume
152
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


The 825–1110 Γ… EUV Spectrum of Venus
✍ S.Alan Stern; David C. Slater; G.Randall Gladstone; Erik Wilkenson; Webster C. C πŸ“‚ Article πŸ“… 1996 πŸ› Elsevier Science 🌐 English βš– 201 KB
Theoretical intensities of Fexivin the s
✍ M. Blaha πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 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

The relative intensities of CI lines in
✍ Carole Jordan πŸ“‚ Article πŸ“… 1967 πŸ› Springer 🌐 English βš– 447 KB

The relative intensity of two CI lines at 1993.6 β€’ and 1657.4 A, observed in the limb spectrum of the sun, is a factor 2.6 β€’ 10 a larger than that expected if both lines were optically thin. It is shown that the observed intensity ratio may be explained in terms of the transfer of photons from 2 165