CHIANTI - an atomic database for emission lines - I. Wavelengths greater than 50 Å
Citations
4,321 citations
2,124 citations
Cites methods from "CHIANTI - an atomic database for em..."
...Over time, the codes used in these papers have been updated or completely rewritten; current versions are the spex code (Kaastra, Mewe & Nieuwenhuijzen 1996) and the chianti code (Dere et al. 1997; Landi et al. 1999)....
[...]
1,781 citations
1,149 citations
1,050 citations
Cites methods from "CHIANTI - an atomic database for em..."
...The response of the EIS instrument to a range of solar conditions has been calculated using synthetic spectra from the CHIANTI data base (Version 4: Dere et al., 1997; Young et al., 2003)....
[...]
References
375 citations
"CHIANTI - an atomic database for em..." refers methods in this paper
...Oscillator strengths and spontaneous transition probabilities (A values) were taken from Wiese et al. (1966) and Martin et al. (1993)....
[...]
...Radiative constants (gf and A values) were taken from Wiese et al. (1966) for dipole transitions....
[...]
116 citations