Ne VII - VERSION 8.0


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

  1. ne_7.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: ne_7.elvlc
    %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
    %observed energy (level 9): Feldman et al., 1997, ApJS, 113, 195
    %Theoretical energy levels (1 - 10): Zhang, Sampson, ADNDT, 1992 , 52, 143
    %theoretical energy levels(11 - 46): Sampson, D.H., Goett, S.J., Clark, R.E.H., 1984, ADNDT, 30, 125
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  K.P. Dere, Jan. 1996
    -1
    
     
    

  3. ne_7.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: ne_7.wgfa
    %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
    %observed energy (level 9): Feldman et al., 1997, ApJS, 113, 195
    %theoretical energy levels: Sampson, D.H., Goette, S.J., Clark, R.E.H., 1984, ADNDT, 30, 125
    %oscillator strengths allowed transitions: Zhang, H., Sampson, D.H., 1992, ADNDT, 52, 43
    %oscillator strengths forbidden transitions: Muhlethaler, Kastner, 1976, A&A, 48, 109
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Enrico Landi and K.P. Dere, Jan 1996
    

  5. ne_7.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: ne_7.splups
    %oscillator strengths: Zhang, H., Sampson, D.H., 1992, ADNDT, 52, 43
    %effective collision strengths: Ramsbottom, Berrington, Bell, 1994, J.Phys.B, 27, L811
    and Ramsbottom, Berrington, Bell, 1995, ADNDT, 61, 105
    %comment: effective collision strengths were provided in the temperature range 3.0 < Log T < 6.4
    %         and have been fitted in the temperature range 4.0 < Log T < 6.4
    %comment: added collisional data for transitions involving level 26. Effects on level populations
    are minimal for electron densities lower than 10^12 cm^-3 (Jun 2003).
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % E. Landi - Jun 2003
    
    

  7. ne_7.psplups (proton collision data)
  8. contains the spline fits to the scaled proton collision strengths.

     
    
    %filename: ne_7.splups
    %rates: Ryans R.S.I., Foster-Woods V.J, Copeland F., Keenan F.P., Matthews A., Reid R.H.G., 1998, ADNDT 70, 179-229
    %energies: CHIANTI database, ver.1, Dere et al., A&AS 125, 149, 1997
    %comment: Fits valid for temperatures 8e4 to 1.5e7 K.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Peter Young  19-Oct-00
    


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

    ne_7_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:28:48 2015