Ar XIII - VERSION 11.0

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

  1. ar_13.elvlc (energy levels)

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

     
 
 Theoretical energies:

Mao, J. , Badnell, N. R., Del Zanna, G., 2020, A&A, 634, A7
DOI:  10.1051/0004-6361/201936931 

Observed energies:

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

Note: for some  levels, the approximate values given by NIST
have not been included.

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


 -1

  2. ar_13.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:

Mao, J. , Badnell, N. R., Del Zanna, G., 2020, A&A, 634, A7
DOI:  10.1051/0004-6361/201936931 

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

gf-values, A-values for the ground configuration 2s2 2p2 and  the 2s 2p3 are from the ab-inition 
MCHF calculation by  G. Tachiev (2004), following 
G. Tachiev and C. Froese Fischer,  (energy adjusted), 2001, Can. J. Phys. 79,955
http://adsabs.harvard.edu/abs/2001CaJPh..79..955T

Observed energies:

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

Note: for some  levels, the approximate values given by NIST
have not been included.

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


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

  3. ar_13.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, July 2020                                        
Produced as part of the 'CHIANTI' atomic data base collaboration by

DOI:  10.1051/0004-6361/201936931                                  
Mao, J. , Badnell, N. R., Del Zanna, G., 2020, A&A, 634, A7        

oscillator strengths and effective collision strengths:

  4. ar_13.psplups (proton collision data)

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

     

%file: ar_13.psplups
%rates: Ryans R.S.I., Foster-Woods V.J, Keenan F.P., Reid R.H.G., 1999, ADNDT 73, 1-42
%energies: CHIANTI database, ver.1, Dere et al., A&AS 125, 149, 1997
%comment: Fits valid for temperatures 6e5 to 4e7 K.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   10-Sep-2002

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

    Page created by Giulio Del Zanna on Tue Dec 3 13:23:11 2024