Fe V - VERSION 8.0


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

  1. fe_5.elvlc (energy levels)
  2. contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.

     
    %filename:  fe_5.elvlc
    %Observed energies: Ralchenko, Yu., Kramida, A.E., Reader, J., and NIST ASD Team (2008). 
           NIST Atomic Spectra Database (version 3.1.5), [Online]. Available: http://physics.nist.gov/asd3 
           [2009, September 1]. National Institute of Standards and Technology, Gaithersburg, MD.
    %Theoretical energies: Ballance, C.P., Griffin, D.C., & McLaughlin, B.M. 2007, J.Phys.B, 40, F327
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %   Peter Young, 3-Sep-2009
     
    

  3. fe_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: fe_5.wgfa
    %Observed energies: Ralchenko, Yu., Kramida, A.E., Reader, J., and NIST ASD Team (2008).
           NIST Atomic Spectra Database (version 3.1.5), [Online]. Available: http://physics.nist.gov/asd3
           [2009, September 1]. National Institute of Standards and Technology, Gaithersburg, MD
    %A-values: Nahar, S.N., Delahaye, F., Pradhan, A.K., Zeippen, C.J., 2000, A&AS, 144, 141
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    %      Peter Young, 2-Sep-2009
    

  5. fe_5.scups (electron collision data)
  6. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).

     
    %filename: fe_5.splups
    %Observed energies: Ralchenko, Yu., Kramida, A.E., Reader, J., and NIST ASD Team (2008). NIST Atomic
    Spectra Database (version 3.1.5), [Online]. Available: http://physics.nist.gov/asd3
    [2009, September 1]. National Institute of Standards and Technology, Gaithersburg, MD.
    %Theoretical energies: Ballance, C.P., Griffin, D.C., & McLaughlin, B.M. 2007, J.Phys.B., 40, F327
    %Comment: The spline fits are accurate to 0.59 % or better over the temeprature range 5000 to 50,000 K.
    % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
    %
    % Peter Young, 2-Sep-2009
    % Peter Young, 22-Sep-2011
    %   - updated fit for transition 1-33 (removed negative spline value)
    
    

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

  8. The html tables below contain the radiative data of the brightest lines sorted in wavelength

    Page created by Giulio Del Zanna on Fri Sep 18 13:27:23 2015