Ne II - VERSION 8.0


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

  1. ne_2.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 (adjusted) energies from 
    D C Griffin, D M Mitnik and N R Badnell 2001 J. Phys. B 34
    
    Produced for the CHIANTI database v.8 by Giulio Del Zanna,  2013 Jun 23
    
     -1
     
    

  3. ne_2.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 (adjusted) energies, gf and A-values:
    D C Griffin, D M Mitnik and N R Badnell 2001 J. Phys. B 34
    
    A-values for a few M1, M2 , E2 forbidden transitions:
    G. Tachiev and C. Froese Fischer, Method: MCHF (ab initio), 2002,
    the MCHF collection at NIST (http://nlte.nist.gov/MCHF/).
    
    Transitions with an A values greater than 10^-5 of the maximum A-value
    were retained.
    
    Produced for the CHIANTI database v.8 by Giulio Del Zanna,  August 2015
    
     
    

  5. ne_2.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    
    
    Data from from
    D C Griffin, D M Mitnik and N R Badnell 2001 J. Phys. B 34
    
    The maximum energy in this calculation was 6 Ry which is
    high enough to generate accurate effective collision strengths up to the
    maximum temperature of 4x10^5 K.
    However, the  collision strengths have been extrapolated to high energies.
    
    Produced for the CHIANTI database v.8 by Giulio Del Zanna,  2013 Jun 23
    
    
    
    

  7. ne_2.psplups (proton collision data)
  8. contains the spline fits to the scaled proton collision strengths.

     
    
    %filename: ne_2.psplups
    %rates: Foster V.J., Keenan F.P., Reid R.H.G., 1994, ADNDT 58, 227
    %energies: Cheng K.T., Kim Y.-K., Desclaux J.P., 1979, ADNDT 24, 111
    %comment: Fit valid for temperatures 5.5e3 to 2e5.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Peter Young   16-May-2001
    


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

    ne_2_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:28:45 2015