P XIV - VERSION 11.0

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

p_14.elvlc (energy levels)

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

 
%filename: p_14.elvlc
%experimental energy levels: Ralchenko Y., Jou, F.C., Kelleher, D.E., Kramida, A.E., Musgrove, A., Reader, J.,
    Wiese, W.L., Olsen, K., 2005, NIST Atomic Spectra Database, Version 3.0
%theoretical energy levels: extrapolated using the ions in the He-like sequence from C V to Ni XXVII
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%  E. Landi - Oct 2004
 -1

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: p_14.wgfa
%experimental energy levels: Ralchenko Y., Jou, F.C., Kelleher, D.E., Kramida, A.E., Musgrove, A., Reader, J.,
    Wiese, W.L., Olsen, K., 2005, NIST Atomic Spectra Database, Version 3.0
%theoretical energy levels: interpolated using the ions in the He-like sequence from C V to Ni XXVII
%A values and oscillator strengths: interpolated using the ions in the He-like sequence from C V to Ni XXVII
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%  E. Landi - Oct 2004
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
%File processed with wgfa_tidy by pryoung on 31-May-2023

p_14.scups (electron collision data)

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

 
%  E. Landi - Oct 2004                                                                                  
%                                                                                                       
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration                 
%comment: the effective collision strengths are most accurate in the range 6.2 < log T < 7.5            
%effective collision strengths: interpolated using the ions in the He-like sequence from C V to Ni XXVII
%oscillator strengths: interpolated using the ions in the He-like sequence from C V to Ni XXVII         
%filename: p_14.splups

(proton collisional data) Not available in this VERSION.

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

p_14_table.html (html table)