Fe VI - VERSION 11.0


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

  1. fe_6.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
     
     Observed energies: Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
    NIST Atomic Spectra Database (ver. 5.0), [Online].
    Available: http://physics.nist.gov/asd [2013, May 3]. 
    National Institute of Standards and Technology, Gaithersburg, MD. 
    
    Theoretical energies:
    Ballance, C. P. & Griffin, D. C. 2008, Journal of Physics B Atomic Molecular Physics, 41, 195205
    
    Produced for the CHIANTI database v.8 by G. Del Zanna Mar 2014
    
     -1
     
    

  3. fe_6.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.

     
    
    Observed energies: Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
    NIST Atomic Spectra Database (ver. 5.0), [Online].
    Available: http://physics.nist.gov/asd [2013, May 3]. 
    National Institute of Standards and Technology, Gaithersburg, MD. 
    
    Theoretical energies, gf and A-values:
    Ballance, C. P. & Griffin, D. C. 2008, Journal of Physics B Atomic Molecular Physics, 41, 195205
    
    A-values for forbidden transitions:
    Chen, G. X. & Pradhan, A. K. 2000, A&AS, 147, 111
    
    
    Produced for the CHIANTI database v.8 by G. Del Zanna Mar 2014
    
     
    %File processed with wgfa_tidy by pryoung on  6-Mar-2019
    %File processed with wgfa_tidy by pryoung on  6-Mar-2019
    %File processed with wgfa_tidy by pryoung on 31-May-2023
    %File processed with wgfa_tidy by pryoung on 31-May-2023
    

  5. fe_6.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 Mar 2014                                  
    
    Ballance, C. P. & Griffin, D. C. 2008, Journal of Physics B Atomic Molecular Physics, 41, 195205
    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 Tue Dec 3 13:24:05 2024