Ni XIV - VERSION 10.1

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

  1. ni_14.elvlc (energy levels)

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

     
%filename: ni_14.elvlc
%observed energy levels (2): Smitt et al. 1976, Phys. Scripta, 13, 293
%observed energy levels (3): Combination of Smitt et al. (1976) and Shirai et al. 2000, J. Phys. Chem. Ref. Data, Mmonograph 8 
%observed energy levels (4): Feldman & Doschek 2007, ADNDT, 93, 779
%observed energy levels (5): Combination of Smitt et al. (1976) and Feldman & Doschek (2007)
%observed energy levels (6): Combination of Fawcett & Hayes (1972) and Borges et al. (2007)
%observed energy levels (7,9,11): Combination of Fawcett & Hayes (1972), Borges et al. (2007), and Shirai et al. (2000)
%observed energy levels (8): Borges et al 2007, Brazilian J. Phys., 37, 335
%observed energy levels (10,12): Combination of Borges et al. (2007) and Shirai et al. (2000)
%observed energy levels (27-31): Fawcett & Hayes 1972, J. Phys. B, 5, 366
%observed energy levels (32,34,39): Combination of Fawcett & Hayes (1972) and ground configuration observed energies
%observed energy levels (36): Combination of Fawcett & Hayes (1972) and Smitt et al. (1976)
%Theoretical energy levels: Landi & Bhatia 2010, ADNDT, 96, 52
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi - Nov 2008

  2. ni_14.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. 

     
%filename: ni_14.wgfa
%observed energy levels (2): Smitt et al. 1976, Phys. Scripta, 13, 293
%observed energy levels (3): Combination of Smitt et al. (1976) and Shirai et al. 2000, J. Phys. Chem. Ref. Data, Mmonograph 8
%observed energy levels (4): Feldman & Doschek 2007, ADNDT, 93, 779
%observed energy levels (5): Combination of Smitt et al. (1976) and Feldman & Doschek (2007)
%observed energy levels (6): Combination of Fawcett & Hayes (1972) and Borges et al. (2007)
%observed energy levels (7,9,11): Combination of Fawcett & Hayes (1972), Borges et al. (2007), and Shirai et al. (2000)
%observed energy levels (8): Borges et al 2007, Brazilian J. Phys., 37, 335
%observed energy levels (10,12): Combination of Borges et al. (2007) and Shirai et al. (2000)
%observed energy levels (27-31): Fawcett & Hayes 1972, J. Phys. B, 5, 366
%observed energy levels (32,34,39): Combination of Fawcett & Hayes (1972) and ground configuration observed energies
%observed energy levels (36): Combination of Fawcett & Hayes (1972) and Smitt et al. (1976)
%Theoretical energy levels: Landi & Bhatia 2010, ADNDT, 96, 52
%A and gf values: Landi & Bhatia 2010, ADNDT, 96, 52
%Comment: A and gf values computed with the Flexible Atomic Code - Gu, M.F., 2003, ApJ, 582, 1241
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi - Nov 2008
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
%File processed with wgfa_tidy by pryoung on 31-May-2023

  3. ni_14.scups (electron collision data)

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

     
% Enrico Landi - Nov 2008
%
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%Collision strengths: Landi & Bhatia, 2010, ADNDT, 96, 52
%gf values: Landi & Bhatia, 2010, ADNDT, 96, 52
%filename: ni_14.splups

  4. (proton collisional data) Not available in this VERSION.

    5. 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 11:18:25 2023