K V - VERSION 8.0


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

  1. k_5.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: k_5.elvlc
    %observed energies: Fuhr, J.R., et al., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data
    %theoretical energies: Wilson, N. J., Bell, K. L. 2001, MNRAS 325, 159
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % P.R. Young - 12 Jun 2002
     
    

  3. k_5.wgfa (radiative data)
  4. 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: k_5.wgfa
    %observed energies: Fuhr, J.R., et al., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data
    %A-values: Mendoza, C., Zeippen, C.J. 1982, MNRAS 198, 127
    %comment: corrected typo for 1-5 transition
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % P.R. Young - 30-Mar-2010
    

  5. k_5.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: k_5.splups
    %theoretical energy levels: Wilson, N. J., Bell, K. L. 2001, MNRAS 325, 159
    %effective collision strengths: Wilson, N. J., Bell, K. L. 2001, MNRAS 325, 159
    %comment: Note that Wilson & Bell only give LS energy levels. The energies
    for the fine structure splittings have been taken from experimental values.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % P.R.Young - 12-Jun-02
    
    

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

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

    k_5_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:28:17 2015