𝔖 Bobbio Scriptorium
✦   LIBER   ✦

ATOMIC DATA AND SPECTRAL LINE INTENSITIES FOR Mg VI

✍ Scribed by A.K. BHATIA; P.R. YOUNG


Publisher
Elsevier Science
Year
1998
Tongue
English
Weight
613 KB
Volume
68
Category
Article
ISSN
0092-640X

No coin nor oath required. For personal study only.

✦ Synopsis


Electron collision strengths for Mg VI, calculated in the distorted-wave approximation, are presented for all transitions between the 23 levels of the 2s 2 2p 3 , 2s2p 4 , 2p 5 , and 2s 2 2p 2 3s configurations. Radiative data have been calculated utilizing the same four-configuration model of the ion. Proton rates for the transitions between the ground states are also presented. The level balance equations for Mg VI have been solved using these data and comparisons are made with previous results-excellent agreement is found. Theoretical line intensities for the important transitions are presented and compared with lines found in the extreme ultraviolet in a spectrum from the 1989 flight of the Solar EUV Rocket Telescope and Spectrograph. Recent data from the Coronal Diagnostic Spectrometer onboard the Solar and Heliospheric Observatory are also presented.


πŸ“œ SIMILAR VOLUMES


ATOMIC DATA AND SPECTRAL LINE INTENSITIE
✍ A.K. BHATIA; G.A. DOSCHEK; W. EISSNER πŸ“‚ Article πŸ“… 2002 πŸ› Elsevier Science 🌐 English βš– 168 KB

Electron impact collision strengths and spontaneous radiative decay rates are calculated for Fe XI. The data pertain to the 96 levels of the configurations 3s 2 3p 4 , 3s3p 5 , 3s 2 3p 3 3d, 3p 6 , 3s 2 3p 3 4s, and 3s 2 3p 3 4d. Collision strengths are calculated at 10 incident electron energies: 1