Ca V - VERSION 8.0


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

  1. ca_5.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: ca_5.elvlc
    %Observed energies: v.3.0.3 of the online NIST database
    %theoretical energies: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347
    %comment: The theoretical energies are from Table 3 of Galavis et al. and are for LS states.
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %   Peter Young   -   9-Jun-2006
     
    

  3. ca_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: ca_5.wgfa
    %Observed energies: v.3.0.3 of the online NIST database
    %A-values: Biemont, E., & Hansen, J.E., 1986, Phys. Scripta, 34, 116
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %   Peter Young   -   9-Jun-2006
    

  5. ca_5.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: ca_5.splups
    %Theoretical energies: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347
    %Upsilons: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347
    %comment: Observed energies used for transitions between levels 1,2 and 3.
    %comment: The original upsilons are valid over the range 10^3 - 10^5 K.  The spline fits reproduce the original upsilons to within 0.38%.
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %    Peter Young  -   9-Jun-2006
    
    

  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

    ca_5_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:25:32 2015