Calculated X-radiation from optically thin plasmas. V

Details Calculated X-radiation from optically thin plasmas. V Calculated X-radiation from optically thin plasmas. V

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...62..197m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 62, Nov. 1985, p. 197-254. Research supported by the Stichti

Astronomy and Astrophysics

Astrophysics

1013

Plasma Radiation, Plasma Spectra, X Ray Spectroscopy, Electron Transitions, Helium Ions, Hydrogen Ions, Iron, Line Spectra, Lithium, Solar Flares, Solar Spectra, Tables (Data)

Scientific paper

The spectral line list in a previously developed computer code has been updated and extended with many new lines up to 300 A. These lines comprise: H- and He-like n = 1-2 lines, together with their satellites which are produced by innershell transitions: 2l-nl-prime (n = 3, 4) transitions in Fe XVII-XXIV (10-17 A); 2s-2p lines in Fe XVIII-XXIII and Ni XX-XXV (90-140 A); 3l-nl-prime (n = 3, 4) transitions in Fe VIII-XVI and Ni X-XIV (50-200 A), and many lines from Li to Ne isoelectronic sequences of elements C to Ca (20-300 A). Intensities of 2131 spectral lines are tabulated over the temperature range 3 x 10 to the 4th - 10 to the 9th K.

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