Chianti-an atomic database for euv emission lines
CHIANTI consists of a critically evaluated set of atomic data and transitionprobabilities necessary to calculate the emission line spectrum of astrophysicalplasmas. The data consist of atomic energy levels, atomic radiative data such aswavelengths, weighted oscillator strengths and A values, and ele...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2000
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57100935 |
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