Ni XV - VERSION 11.0

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

  1. ni_15.elvlc (energy levels)

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

     
 
  Observed energies: Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
NIST Atomic Spectra Database (ver. 5.0), [Online].
Available: http://physics.nist.gov/asd [2013, May 3]. 
National Institute of Standards and Technology, Gaithersburg, MD. 

Note: some energies have been added/revised in 
Del Zanna, G., Storey, P.J., Mason, H.E., 2014, A&A, in press


Theoretical energies:
Del Zanna, G., Storey, P.J., Mason, H.E., 2014, A&A, in press

Produced for the CHIANTI database v.8 by G. Del Zanna June 2014

 -1

  2. ni_15.wgfa (radiative data)

    3. 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 energies: Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). 
NIST Atomic Spectra Database (ver. 5.0), [Online].
Available: http://physics.nist.gov/asd [2013, May 3]. 
National Institute of Standards and Technology, Gaithersburg, MD. 

Note: some energies have been added/revised in 
Del Zanna, G., Storey, P.J., Mason, H.E., 2014, A&A, in press


Theoretical energies, gf and A-values:
Del Zanna, G., Storey, P.J., Mason, H.E., 2014, A&A, in press

Produced for the CHIANTI database v.8 by G. Del Zanna June 2014
 
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
%File processed with wgfa_tidy by pryoung on 31-May-2023

  3. ni_15.scups (electron collision data)

    4. contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992). 

     

 Produced for the CHIANTI database v.8 by G. Del Zanna June 2014       


Data from Del Zanna, G., Storey, P.J., Mason, H.E., 2014, A&A, in press

  4. ni_15.psplups (proton collision data)

    5. contains the spline fits to the scaled proton collision strengths. 

     

%file: ni_15.psplups
%rates: Faucher, P. 1977, A&A 54, 589
%energies: Faucher, P. 1977, A&A 54, 589
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   13-Dec-2001

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

    Page created by Giulio Del Zanna on Tue Dec 3 13:24:47 2024