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

o_3.elvlc (energy levels)

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

 
%energy levels (n=2): Edlen, B., 1985, Phys.Scripta, 31, 345
%energy levels (n=3): Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995, 
   NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61.
%Theoretical energy levels configurations 2s2.2p2, 2s.2p3, 2p4: Aggarwal, K.M., ApJSS, 52, 387, 1983
%Theoretical energy levels other configurations: Bhatia, A.K., Kastner, S.O., 1993, ADNDT, 54,133
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%  E. Landi 2000
 

o_3.wgfa (radiative data)

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 energy levels (n=2): Edlen, B., 1985, Phys.Scripta, 31, 345
%observed energy levels (n=3): Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995,
   NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61
%oscillator strengths: Bhatia, A.K., Kastner, S.O., 1993, ADNDT, 54, 133
%A-values (2-4 and 3-4 transitions): Storey PJ, Zeippen CJ, MNRAS 312, 813, 2000
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Enrico Landi and P.R. Young, 2000

o_3.splups (electron collision data)

contains the spline fits to the electron collision strengths scaled according the rules formulated by Burgess and Tully (1992). Accurate replication of the temperature averaged collision strength over a wide range of temperatures can be accomplished with the data in this file.

 

%filename: o_3.splups
%oscillator strengths: Bhatia, A.K., Kastner, S.O., 1993, ADNDT, 54, 133
%effective collision strengths (trans. within 2s2.2p2 levels): Burke, V.M., Lennon, D.J., 1994, A&ASS, 103, 273
%effective collision strengths for most of the transitions between 2s2.2p2, 2s.2p3, 2p4 levels: 
     Aggarwal, K.M., ApJSS, 1983, 52, 387 and  Aggarwal, K.M., A&A, 1985, 146, 149
%collision strengths all other transitions: Bhatia, A.K., Kastner, S.O., 1993, ADNDT, 54, 133
%comment: effective collision strengths are accurate in the temperature range 3.7 < Log T < 5.0
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%E.Landi and K.P.Dere 1996

o_3.psplups (proton collision data)

contains the spline fits to the scaled proton collision strengths.

 

%file: o_3.psplups
%rates: Ryans R.S.I., Foster-Woods V.J, Keenan F.P., Reid R.H.G., 1999, ADNDT 73, 1-42
%energies: Wiese W.L., Fuhr J.R., Deters T.M., 1996, J. Phys. Chem. Ref. Data, Monograph 7
%comment: Fits valid for temperatures 1.5e4 to 2e6 K.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   15-May-2001

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

o_3_table.html (html table)


Last revised by G. Del Zanna on 4-Sep-2009