K XV - VERSION 10.0.2


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

  1. k_15.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
     
     Experimental energies:
    Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2013).
    NIST Atomic Spectra Database (ver. 5.1), see http://physics.nist.gov/asd
    
    Note: levels 3,4,5, 11, 50,51  have an observed enrgy only known relative 
    to that of other levels.
    
    
    
    Theoretical energies:
    G Y Liang, N R Badnell and G Zhao  A&A 547, A87 (2012)
       DOI: 10.1051/0004-6361/201220277
    
     Produced for the CHIANTI database v.8 by G. Del Zanna 28 Apr 2014
    
     -1
     
    

  3. k_15.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.

     
    
    Experimental energies:
    Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2013).
    NIST Atomic Spectra Database (ver. 5.1), see http://physics.nist.gov/asd
    
    Note: levels 3,4,5, 11, 50,51  have an observed enrgy only known relative 
    to that of other levels.
    
    
    Theoretical energies, gf and A-values:
    G Y Liang, N R Badnell and G Zhao  A&A 547, A87 (2012)
       DOI: 10.1051/0004-6361/201220277
    
    Note: only transitions with a branching ratio above 10^-5 
    have been retained.
    
    Transitions within the first 15 levels (2s 2p2, 2p3):
    P. Rynkun, P. Jonsson, G. Gaigalas,  C. Froese Fischer
    Atomic Data and Nuclear Data Tables 98 (2012) 481, 556
    
     Produced for the CHIANTI database v.8 by G. Del Zanna 10 Nov 2014
     
    
    
     
    %File processed with wgfa_tidy by pryoung on  6-Mar-2019
    

  5. k_15.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    
    Produced for the CHIANTI database v.8 by G. Del Zanna 10 Nov 2014
    
    Note: data for levels 8,9 have been corrected.
    
       DOI: 10.1051/0004-6361/201220277
    G Y Liang, N R Badnell and G Zhao  A&A 547, A87 (2012)
     Data from 
     
    

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

  8. The html tables below contain the radiative data of the brightest lines sorted in wavelength

    Page created by Giulio Del Zanna on Wed Jun 8 16:07:02 2022