1988
DOI: 10.1007/bf01384442
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Beam-foil spectroscopy in the 3–6 nm soft-X-ray range

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Cited by 14 publications
(5 citation statements)
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“…The density sensitivity of the Mg IX lines is moderate at typical active region densities, and intensity ratios among lines from the 2s2p 3 P-2p 2 3 P multiplet can be used to measure plasma electron densities N e only below 10 9 cm À3 , so that only in quiet Sun conditions and outside the solar disk Table B Comparison between lifetimes (in 10 À10 s units) predicted by the present calculations and measured by Granzow et al [13] (G94), Träbert and Heckmann [11] (TH80), and Mö ller et al [12] can Mg IX lines be used for density diagnostics. Such ratios are density sensitive also for N e > 10 12 cm À3 , however, such densities are typical of flare plasmas, where temperature is much higher than the temperature range where Mg IX is formed, so this density dependence cannot be used for diagnostics.…”
Section: Diagnostic Relevance Of the N = 3 And N = 4 Transitionsmentioning
confidence: 95%
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“…The density sensitivity of the Mg IX lines is moderate at typical active region densities, and intensity ratios among lines from the 2s2p 3 P-2p 2 3 P multiplet can be used to measure plasma electron densities N e only below 10 9 cm À3 , so that only in quiet Sun conditions and outside the solar disk Table B Comparison between lifetimes (in 10 À10 s units) predicted by the present calculations and measured by Granzow et al [13] (G94), Träbert and Heckmann [11] (TH80), and Mö ller et al [12] can Mg IX lines be used for density diagnostics. Such ratios are density sensitive also for N e > 10 12 cm À3 , however, such densities are typical of flare plasmas, where temperature is much higher than the temperature range where Mg IX is formed, so this density dependence cannot be used for diagnostics.…”
Section: Diagnostic Relevance Of the N = 3 And N = 4 Transitionsmentioning
confidence: 95%
“…The incident electron energies were chosen to encompass a wide range spanning from threshold to high energies. For transitions from within the ground configuration levels to the first 10 levels (n = 2 configurations) we calculated collision strengths at 6,12,25,50,75, 100, and 125 Ry, since the excitation energies of these transitions are lower than 5 Ry. Collision strengths for transitions between the ground configuration and the n = 3, 4, 5 configurations were calculated at 25, 50, 75, 100, and 125 Ry, since the excitation energies of these transitions are in the 11.4-20.9 Ry energy range.…”
Section: Atomic Datamentioning
confidence: 99%
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