The CHIANTI database has the following primary ASCII files for this ion:

- zn_28.elvlc (energy levels)
- zn_28.wgfa (radiative data)
- zn_28.scups (electron collision data)
- (proton collisional data) Not available in this VERSION.

contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

%filename: zn_28.elvlc Theoretical energy levels: Autostructure calculation A Breit-Pauli distorted wave implementation for AUTOSTRUCTURE Badnell, N.R., 2011, Computer Physics Communications, 182, 1528 ADSref: http://adsabs.harvard.edu/abs/2011CoPhC.182.1528B Autostructure calculation optimized with 'SHFTIC' file using energy corrections from the following sources: observed(theoretical) energies for n=2 above IP Yerokhin, V. A.; Surzhykov, A., Physical Review A, vol. 86, Issue 4, id. 042507 Relativistic configuration-interaction calculation of energy levels of core-excited states in lithiumlike ions: Argon through krypton ADSref: http://adsabs.harvard.edu/abs/2012PhRvA..86d2507Y DOI: http://dx.doi.org/10.1103/PhysRevA.86.042507 Theoretical energies for n=3 above IP Goryaev, F. F.; Vainshtein, L. A.; Urnov, A. M. Atomic data for doubly-excited states 2lnl‧ of He-like ions and 1s2lnl‧ of Li-like ions with Z = 6-36 and n = 2 , 3 2017, ADNDT, 113, 117-257 adsRef: http://adsabs.harvard.edu/abs/2017ADNDT.113..117G DOI: 10.1016/j.adt.2016.04.002 Theoretical energy levels (n=4,5 above IP): calculations of U. Safronova reported in Kato et al., 1997, ADNDT, 67, 225. ADS http://adsabs.harvard.edu/abs/1997ADNDT..67..225K updated by U. Safronova, 2001, private communication produced as a part of the 'CHIANTI' atomic database for astrophysical spectroscopy K. Dere (GMU) - 2018 December 01 zn_28 IP ev = 2.78345e+03 Ip invcm = 22450000.000 Ip Ryd = 204.57945 zn_29 IP ev = 1.18648e+04 Ip invcm = 95696100.000 Ip Ryd = 872.04700

contains wavelengths, gf and A values of the transitions. The wavelengths are based on the experimental energy levels and should be the best available. Wavelengths calculated from the theoretical energies are of an indeterminate accuracy and their values are presented as negative values of the calculated wavelength.

%filename: zn_28.wgfa Theoretical gf and A-values: Autostructure calculation A Breit-Pauli distorted wave implementation for AUTOSTRUCTURE Badnell, N.R., 2011, Computer Physics Communications, 182, 1528 ADSref: http://adsabs.harvard.edu/abs/2011CoPhC.182.1528B Autostructure calculation optimized with 'SHFTIC' file using energy corrections from the following sources: observed(theoretical) energies for n=2 above IP Yerokhin, V. A.; Surzhykov, A., Physical Review A, vol. 86, Issue 4, id. 042507 Relativistic configuration-interaction calculation of energy levels of core-excited states in lithiumlike ions: Argon through krypton ADSref: http://adsabs.harvard.edu/abs/2012PhRvA..86d2507Y DOI: http://dx.doi.org/10.1103/PhysRevA.86.042507 Theoretical energies for n=3 above IP Goryaev, F. F.; Vainshtein, L. A.; Urnov, A. M. Atomic data for doubly-excited states 2lnl‧ of He-like ions and 1s2lnl‧ of Li-like ions with Z = 6-36 and n = 2 , 3 2017, ADNDT, 113, 117-257 adsRef: http://adsabs.harvard.edu/abs/2017ADNDT.113..117G DOI: 10.1016/j.adt.2016.04.002 Theoretical energy levels (n=4,5 above IP): calculations of U. Safronova reported in Kato et al., 1997, ADNDT, 67, 225. ADS http://adsabs.harvard.edu/abs/1997ADNDT..67..225K updated by U. Safronova, 2001, private communication Wavelengths determined from energy levels Minimum branching ratio = 1.00e-04 allWvl = 1 minDiff = 0.00010 outfile = zn_28.wgfa.olg.imp produced as a part of the 'CHIANTI' atomic database for astrophysical spectroscopy K. Dere (GMU) - 2018 December 02 %File processed with wgfa_tidy by pryoung on 6-Mar-2019

contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

K. Dere (GMU) - 2013 January 03 produced as a part of the 'CHIANTI' atomic database for astrophysical spectroscopy collision strengths provided in the range 1.57e+05 to 1.57e+09 K ADS ref: https://ui.adsabs.harvard.edu/abs/2011A%26A...528A..69L/abstract DOI: https://ui.adsabs.harvard.edu/link_gateway/2011A&A...528A..69L/doi:10.1051/0004-6361/201016417 Astronomy & Astrophysics, Volume 528, id.A69, 15 pp including Auger and radiation damping R-matrix electron-impact excitation data for the Li-like iso-electronic sequence Liang, G. Y.; Badnell, N. R. Theoretical collision strengths: %filename: zn_28.upsdat

* Page created by Giulio Del Zanna on Wed Jun 8 16:15:38 2022*