S V - VERSION 10.1

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

  1. s_5.elvlc (energy levels)

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

     
 


Theoretical energies:
Fernandez-Menchero, L., Del Zanna, G. and Badnell, N.R.
A&A, 2014, 572, A115
doi = {10.1051/0004-6361/201424849

Note: only  bound levels have been retained.

Observed energies: NIST Atomic Spectra Database, (ver. 5.7.1), [Online].
https://physics.nist.gov/PhysRefData/ASD/levels_form.html


Produced as part of the 'CHIANTI' atomic data base collaboration by
Giulio Del Zanna, May 2020

 -1

  2. s_5.wgfa (radiative data)

    3. 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. 

     

gf-values, A-values and theoretical energies:
Fernandez-Menchero, L., Del Zanna, G. and Badnell, N.R.
A&A, 2014, 572, A115
doi = {10.1051/0004-6361/201424849

Only transition probabilities with a branching ratio
greater than 10^(-5) have been retained.

Note: only  bound levels have been retained.

gf-values, A-values for the n=3 (lowest 26 levels):
MCHF calculation by
G. Tachiev and C. Froese Fischer, Method: MCHF (ab initio), 2002
https://nlte.nist.gov/MCHF/periodic.html

Observed energies: NIST Atomic Spectra Database, (ver. 5.7.1), [Online]
https://physics.nist.gov/PhysRefData/ASD/levels_form.html


Produced as part of the 'CHIANTI' atomic data base collaboration by
Giulio Del Zanna, May 2020

 
%File processed with wgfa_tidy by pryoung on 31-May-2023

  3. s_5.scups (electron collision data)

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

     

Giulio Del Zanna, May 2020
Produced as part of the 'CHIANTI' atomic data base collaboration by

Note: only  bound levels have been retained.

doi = {10.1051/0004-6361/201424849
A&A, 2014, 572, A115
Fernandez-Menchero, L., Del Zanna, G. and Badnell, N.R.

oscillator strengths and effective collision strengths:

  4. s_5.psplups (proton collision data)

    5. contains the spline fits to the scaled proton collision strengths. 

     

%filename: s_5.psplups
%rates: Landman, D.A., Brown, T., 1979, ApJ 232, 636
%energies: Observed energies from CHIANTI .elvlc file.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   18-May-2001

    The html tables below contain the radiative data of the brightest lines sorted in wavelength

    Page created by Giulio Del Zanna on Mon Jun 26 11:19:22 2023