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A comparison of theoretical Sv emission line strengths with extreme ultraviolet observations of a sunspot

โœ Scribed by F. P. Keenan; J. G. Doyle


Book ID
104966324
Publisher
Springer
Year
1990
Tongue
English
Weight
333 KB
Volume
128
Category
Article
ISSN
0038-0938

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A comparison of theoretical Oiiiline str
โœ F. P. Keenan; S. M. McCann; K. M. Aggarwal; K. G. Widing ๐Ÿ“‚ Article ๐Ÿ“… 1989 ๐Ÿ› Springer ๐ŸŒ English โš– 288 KB

Relative level populations in OIII, determined using R-matrix calculations of electron impact excitation rates, are used to derive the theoretical emission line ratios R 1 = 1(525.80 ~)/I(599.62 A), R 2 = I(507.41 h)/I(599.62 A), R3 = 1(507.71 A)/I(599.62/~), and R4 = 1(508.18 A)/I(599.62 it). Elect