Ni XII - VERSION 11.0

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

  1. ni_12.elvlc (energy levels)

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

     

Theoretical energies:

Del Zanna, G., & Badnell, N. R. 2016, A&A, 585, A118
 doi = 10.1051/0004-6361/201527378

Note: only the lowest 589 states have been retained.

 Observed energies:

As discussed by
Del Zanna, G., & Badnell, N. R. 2016, A&A, 585, A118
and revised by 
Wang, K., Jönsson, P., Del Zanna, G., et al. 2020, ApJS, 246, 1
 doi = 10.3847/1538-4365/ab5530

Produced for the CHIANTI database v.10 by Giulio Del Zanna, Sept 2020


 -1

  2. ni_12.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. 

     

Theoretical energies, gf and A-values:

Del Zanna, G., & Badnell, N. R. 2016, A&A, 585, A118
 doi = 10.1051/0004-6361/201527378

Note: only the lowest 589 levels have been retained.


Observed energies:

As discussed by
Del Zanna, G., & Badnell, N. R. 2016, A&A, 585, A118
and revised by 
Wang, K., Jönsson, P., Del Zanna, G., et al. 2020, ApJS, 246, 1
 doi = 10.3847/1538-4365/ab5530

Produced for the CHIANTI database v.10 by Giulio Del Zanna, Sept 2020


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

  3. ni_12.scups (electron collision data)

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

     



Produced for the CHIANTI database v.10 by Giulio Del Zanna, Sept 2020


Note: only the lowest 589 states have been retained.                 


 doi = 10.1051/0004-6361/201527378                                   
Del Zanna, G., & Badnell, N. R. 2016, A&A, 585, A118                 

Rates from

  4. ni_12.psplups (proton collision data)

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

     

%filename: ni_12.psplups
%rates: Bely, O., Faucher, P., 1970, A&A 6, 88
%energies: Observed energies from .elvlc file.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   11-Jun-2001

    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 13:24:46 2024