Dielectronic Recombination Rate Coefficients for H-like through Ne-like Isosequences of Mg, Si, S, Ar, Ca, Fe, and Ni
By M. Gu. 2003
167 citations recorded by the source corpus.
Subfields: Atomic and Molecular Physics, and Optics, Mechanics of Materials
View Paper: https://www.semanticscholar.org/paper/0cce6233d01407a5af700ed0f4f2dcb86081fb78
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In Atomic and Molecular Physics, and Optics
In Mechanics of Materials
Citations in the corpus
- A NEW APPROACH TO ANALYZING SOLAR CORONAL SPECTRA AND UPDATED COLLISIONAL IONIZATION EQUILIBRIUM CALCULATIONS. II. UPDATED IONIZATION RATE COEFFICIENTS (2008, background): “Recently, however, state-of-the-art electron-ion recombina- tion data have been published for K-shell, L-shell, and Na-like ions of all elements from H – 3 – through Zn (Badnell et al. 2003; Badnell 2006a,b,c; Gu 2003a,b, 2004).”
- Multidimensional modelling of X-ray spectra for AGN accretion disc outflows (2008, methodology): “Radiative recombination rates are taken from Gu (2003b), where available, or else from Verner & Ferland (1996) (H-, Heand Li-like ions of C, N, O and Ne and Na-like ions of Fe and Ni), Arnaud & Raymond (1992) (FeXVI ) or Shull & van Steenberg (1982b,a), otherwise.”
- UPDATED ATOMIC DATA AND CALCULATIONS FOR X-RAY SPECTROSCOPY (2012, background): “Calculations of DR rate coefficients by Badnell (2006a) and Gu (2003a, 2004) agree to within 35% of each other.”