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Title:
Calculated X-radiation from optically thin plasmas. V
Authors:
Mewe, R.; Gronenschild, E. H. B. M.; van den Oord, G. H. J.
Affiliation:
AA(Laboratorium voor Ruimteonderzoek, Utrecht, Netherlands), AB(Laboratorium voor Ruimteonderzoek, Utrecht, Netherlands), AC(Sterrewacht Sonnenborgh, Utrecht, Netherlands)
Publication:
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 62, Nov. 1985, p. 197-254. Research supported by the Stichting Astronomisch Onderzoek in Nederland and ZWO. (A&AS Homepage)
Publication Date:
11/1985
Category:
Plasma Physics
Origin:
STI
NASA/STI Keywords:
PLASMA RADIATION, PLASMA SPECTRA, X RAY SPECTROSCOPY, ELECTRON TRANSITIONS, HELIUM IONS, HYDROGEN IONS, IRON, LINE SPECTRA, LITHIUM, SOLAR FLARES, SOLAR SPECTRA, TABLES (DATA)
Bibliographic Code:
1985A&AS...62..197M

Abstract

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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