Ti XI - VERSION 8.0


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

  1. ti_11.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: ti_11.elvlc
    %experimental energy levels: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995,
       NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61.
    %theoretical energy levels: interpolated using Si III, S V, Ar VII, Ca IX, Cr XIII, Ni XVII.
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Enrico Landi 1997
     
    

  3. ti_11.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: ti_11.wgfa
    %observed energy levels: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995,
        NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61.
    % Radiative transitions prob.: interpolated using Si III, S V, Ar VII, Ca IX, Cr XIII, Ni XVII.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Enrico Landi 1997
    

  5. ti_11.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: ti_11.splups
    %oscillator strengths: interpolated using Si III, S V, Ar VII, Ca IX, Cr XIII, Ni XVII
    %effective collision strengths: interpolated using Si III, S V, Ar VII, Ca IX, Cr XIII, Ni XVII
    %comment: the quality of the effective collision strengths is not very high due to strange features
    along the isoelectronic sequence.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Enrico Landi 1997
    
    

  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

    ti_11_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:29:47 2015