S VII - VERSION 11.0

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

s_7.elvlc (energy levels)

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

 
 
Observed energies: 
Mostly from 
Jupen C. and Engstrom L., 2002, Physica Scripta, 66, 140

Those for levels 6,69, 93, 113, 143,147,177 
are from Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
NIST Atomic Spectra Database (ver. 5.0), [Online]. Available: http://physics.nist.gov/
  
Theoretical energies: 
 Liang, G. Y. & Badnell, N. R. 2010, A&A, 518, A64
 doi = {10.1051/0004-6361/201014170}
 adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...518A..64L}

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:  ./s_7.wgfa

Observed energies:
Mostly from
Jupen C. and Engstrom L., 2002, Physica Scripta, 66, 140

Those for levels 6,69, 93, 113, 143,147,177
are from Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012).
NIST Atomic Spectra Database (ver. 5.0), [Online]. Available: http://physics.nist.gov/

Theoretical energies, gf and A-values:
Liang, G. Y. & Badnell, N. R. 2010, A&A, 518, A64
doi = {10.1051/0004-6361/201014170}
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...518A..64L}

Note: only transitions with a branching ratio above 10^-5
have been retained.

Transitions within the first 27 levels (2p6, 2p5 3l, l=s,p,d):
Jonsson P. et al., Atomic Data and Nuclear Data Tables, 2014, 100, 1
adsurl = {http://adsabs.harvard.edu/abs/2014ADNDT.100....1J}

Produced for the CHIANTI database v.8 by G. Del Zanna 9 Mar 2015

 K. Dere  -  minimum branching ratio =   1.00e-05  :  2017 December 15
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
%File processed with wgfa_tidy by pryoung on 31-May-2023

s_7.scups (electron collision data)

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

 

Produced for the CHIANTI database v.8 by Giulio Del Zanna  Nov 2013 
                                                                    
                                                                    
      adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...518A..64L}
      doi = {10.1051/0004-6361/201014170}                           
Data from Liang, G. Y. & Badnell, N. R. 2010, A&A, 518, A64

(proton collisional data) Not available in this VERSION.

The html table below contains the radiative data of the brightest lines sorted in wavelength

s_7_table.html (html table)