Ne VI - VERSION 11.0

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

  1. ne_6.elvlc (energy levels)

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

     
 
Experimental energies:
Kramida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2013).
NIST Atomic Spectra Database (ver. 5.1), see http://physics.nist.gov/asd


Theoretical energies:
G Y Liang, N R Badnell and G Zhao  A&A 547, A87 (2012)
   DOI: 10.1051/0004-6361/201220277

Note: in the previous v.8 file levels 6,7
an 12, 13  were inverted. 

  Produced for the CHIANTI database  by G. Del Zanna 7 August 2017

% 23-Oct-2020, Peter Young
  Removed level 204 (2s 2p 4f 2D3/2) as the collision strengths for this levels
  are all zero.

 -1

  2. ne_6.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. 

     

Theoretical energies, gf and A-values:

G Y Liang, N R Badnell and G Zhao  A&A 547, A87 (2012)
   DOI: 10.1051/0004-6361/201220277


Transitions within the first 15 levels (2s 2p2, 2p3):
P. Rynkun, P. Jonsson, G. Gaigalas,  C. Froese Fischer
Atomic Data and Nuclear Data Tables 98 (2012) 481 1556

Note: the previous v.8 file had incorrect values for the 
transitions from levels 6,7 which were inverted. 

Note: only transitions with a branching ratio above 10^-5 
have been retained.

Produced for the CHIANTI database  by G. Del Zanna 7 Aug 2017
 
%File processed with wgfa_tidy by pryoung on  6-Mar-2019

%Peter Young, 28-Oct-2020
  - removed level 204 from this file as the collision strengths for this level
    are all zero. 
%File processed with wgfa_tidy by pryoung on 31-May-2023

  3. ne_6.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  by G. Del Zanna 12 Jun 2017
transitions from levels 6,7 which were inverted.               
Note: the previous v.8 file had incorrect values for the       
   DOI: 10.1051/0004-6361/201220277                            
G Y Liang, N R Badnell and G Zhao  A&A 547, A87 (2012)         
Data are from

  4. ne_6.psplups (proton collision data)

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

     

%filename: ne_6.psplups
%rates: Foster VJ, Keenan FP, Reid RHG, ADNDT 67, 99, 1997
%energies: From .elvlc file, experimental energies
%comment: The rate coefficients are in units cm^3/s.
%comment: Fits valid for temperatures 6e4 to 1e6 K.
%produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% Peter Young   15-May-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 13:24:31 2024