O V - VERSION 8.0


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

  1. o_5.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: o_5.elvlc
    %observed energies (n=2,3): NIST Atomic Spectra Database, 2012, V.5, NIST Standard Reference Database 78
    %observed energies (n=4,5): Moore, C.E. 1993, "Tables of spectra of Hydrogen, Carbon, Nitrogen, and Oxygen atoms and
     ions", Edited by J.W. Gallager, CRC Press
    % Theoretical energy levels: Bhatia & Landi, 2012, ADNDT, in press
    %produced as part of the Arcetri/Cambridge/NRL CHIANTI atomic data base collaboration
    %
    % Enrico Landi - Aug 2012
     
    

  3. o_5.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: o_5.wgfa
    %observed energies (n=2,3): NIST Atomic Spectra Database, 2012, V.5, NIST Standard Reference Database 78
    %observed energies (n=4,5): Moore, C.E. 1993, "Tables of spectra of Hydrogen, Carbon, Nitrogen, and Oxygen atoms and ions", Edited by J.W. Gallager, CRC Press
    %Theoretical energy levels: Bhatia & Landi, 2012, ADNDT, in press
    %A and gf values: Bhatia & Landi, 2012, ADNDT, in press
    %produced as part of the Arcetri/Cambridge/NRL CHIANTI atomic data base collaboration
    %
    % Enrico Landi - Aug 2012
    

  5. o_5.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: o_5.splups
    %Theoretical energies (n=2,3): Berrington, K.A., private communication, 13-Mar-03
    %Theoretical energies (n=4,5): Bhatia & Landi, 2012, ADNDT, in press
    %gf-values (n=2,3): Berrington, K.A., private communication, 13-Mar-03
    %Oscillator strengths (n=4,5): Bhatia & Landi, 2012, ADNDT, in press
    %upsilons (n=2,3): Berrington, K.A., private communication, 13-Mar-03
    %Collision strengths (n=4,5): Bhatia & Landi, 2012, ADNDT, in press
    %comment: This data is from the same calculation as presented in
    Kato et al. 1990, ADNDT, 44, 133 but contains more levels
    and some errors in the original paper have been corrected.
    %comment: the fits are accurate in the range 4.2 < log T < 6.3
    %comment: The original data were tabulated over the logT range 3.5 to 6.5,
    however for many transitions it was not possible to get a
    good fit over the whole range. The fits are accurate to <2%
    %
    % Enrico Landi and Peter Young - April 9, 2012
    
    

  7. o_5.psplups (proton collision data)
  8. contains the spline fits to the scaled proton collision strengths.

     
    
    %file:  o_5.psplups
    %prepared for the CHIANTI database by Peter Young, 5-Dec-2014
          contact: pyoung9@gmu.edu
    %rates:
           Ryans R.S.I., Foster-Woods V.J, Copeland F., Keenan F.P.,
           Matthews A., Reid R.H.G., 2000,
           ADNDT 70, 179-229
    %energies:
           Wiese W.L., Fuhr J.R., Deters T.M., 1996,
           J. Phys. Chem. Ref. Data, Monograph #7
    %comments:
      The fits are accurate to < 1.3% over the temperature range 6x10^4 to 2x10^7 K. 
    


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

    o_5_table.html (html table)

    Page created by Giulio Del Zanna on Fri Sep 18 13:29:23 2015