H I - VERSION 10.1


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

  1. h_1.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename: h_1.elvlc
    %observed energy levels: Fuhr et al, 1999, NIST Atomic Spectra Database Version 2.0
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  Ken Dere  May 3 2001
     
    

  3. h_1.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: h_1.wgfa
    % observed energy levels: Fuhr et al, 1999, NIST Atomic Spectra Database Version 2.0,
    %oscillator strengths: Wiese,W.L., Smith,M.W., Glennon,B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4
    % A values (1s-2s): Parpia,F.A., Johnson,W.R., 1982, Phys.Rev.A, 26, 1142.
    %comment: Wavelengths have been calculated the original energy levels from NIST, that include more
              decimal figures than allowed by CHIANTI format.
    %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %  Ken Dere  May 2001
    %File processed with wgfa_tidy by pryoung on  6-Mar-2019
    %File processed with wgfa_tidy by pryoung on 31-May-2023
    

  5. h_1.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
      compiled by Ken Dere (NRL)  Thu Feb  7 15:11:55 2002
    %note:  fine structure collision assumes LS coupling or distribution according to statistical weights
    %collision strengths:  Anderson, H., Ballance, C.P., Badnell, N.R., Summers, H.P., 2000, J. Phys. B, 33,1255, revised 2002
    %note:  hydrogenic f values
     Atomic Transition Probabilities, NSRDS-NBS-4.
    %oscillator strengths:  Wiese, W. L., Smith, M. W., and Glennon, B. M., 1966,
      http://physics.nist.gov/cgi-bin/AtData/main_asd
    %energy levels:    NIST Atomic Spectra Database Version 2.0
      Ken Dere   Wed Jul 26 08:24:54 2000
     collaboration 'CHIANTI' 
    %produced as part of the Arcetri/Cambridge/NRL atomic data base
    % A values:  Parpia, F. A., and Johnson, W. R., 1972, Phys. Rev. A, 26, 1142.
    % produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration
    

  7. (proton collisional data) Not available in this VERSION.

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

    h_1_table.html (html table)

    Page created by Giulio Del Zanna on Mon Jun 26 11:17:00 2023