The CHIANTI database has the following primary ASCII files for this ion:
contains the energy levels (in cm-1). It includes both experimental and theoretical values of the levels energies.
%filename: si_7.elvlc
%observed energy levels (n=2): Edlen, B. 1983, Physica Scripta, 28, 51
%observed energy levels (12,19,23-26,65-67,69,70,72-74,78-82,84,85): Fuhr, J.R., et al.,
"NIST Atomic Spectra Database" ver. 2.0 March 1999. NIST Physical Reference Data
%observed energy levels (16-18,20,21,29,31-34,40-42,46,48,52,55,57,59,62,63): Kink, I., Jupen, C.,
Engstroem, L., Feldman, U., Laming, J.M., Schuehle, U., 1997, ApJ, 487, 956
%observed energy levels (11,13-15,22,28,30,35-37,43-45,47,49-51,53,54,56,60,61,64,68,71,75-77,86):
Kink, I., Engstroem, L., 1997, Physica Scripta, 56, 31
%theoretical energy levels: From the 24-configuration model by Bhatia, A.K., Landi, E., 2003, ApJ, 585, 587
% Comment: The observed energy of level 11 is in reality theoretical. It has been inserted so that
energies of levels 16,17,18 could be determined from its value and the experimental
energy difference measured by Kink et al 1997 from transitions involving each of these levels
with level 11. The energy of levels 40,41,42 has then been determined from the energy difference
measured by Kink et al 1997 for the transitions between levels 16-18 and 40-42.
This means that the absolute energies of levels 16,17,18,40,41,42 are probably offset by
a constant value, but their energy difference is experimentally correct. This allows
CHIANTI to correctly calculate the transition wavelengths from these levels, to reproduce
lines observed by SUMER in solar active and quiet spectra.
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Jan 2009
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: si_7.wgfa %observed energy levels (n=2): Edlen, B. 1983, Physica Scripta, 28, 51 %observed energy levels (12,19,23-26,65-67,69,70,72-74,78-82,84,85): Fuhr, J.R., et al., "NIST Atomic Spectra Database" ver. 2.0 March 1999. NIST Physical Reference Data %observed energy levels (16-18,20,21,29,31-34,40-42,46,48,52,55,57,59,62,63): Kink, I., Jupen, C., Engstroem, L., Feldman, U., Laming, J.M., Schuehle, U., 1997, ApJ, 487, 956 %observed energy levels (11,13-15,22,28,30,35-37,43-45,47,49-51,53,54,56,60,61,64,68,71,75-77,86): Kink, I., Engstroem, L., 1997, Physica Scripta, 56, 31 %theoretical energy levels: From the 24-configuration model by Bhatia, A.K., Landi, E., 2003, ApJ, 585, 587 %Radiative data: From the 24-configuration model by Bhatia, A.K., Landi, E., 2003, ApJ, 585, 587 %Radiative data transition within the ground configuration: Tachiev, G.I., Froese Fischer, C., 2002, A&A, 385, 716 %Radiative data 3-4 and 4-5 transitions: Froese Fischer, C., Saha, H.P., 1983, Phys. Rev. A., 28, 3169 % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi - Jan 2009 K. Dere - minimum branching ratio = 1.00e-05 2017 December 06 %File processed with wgfa_tidy by pryoung on 6-Mar-2019
contains the effective electron collision strengths scaled according to the rules formulated by Burgess and Tully (1992).
% E. Landi - Oct 2002 % % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration %collision strengths: Bhatia, A.K., Landi, E., 2003, ApJ, 585, 587 %oscillator strengths: Bhatia, A.K., Landi, E., 2003, ApJ, 585, 587 %filename: si_7.splups
contains the spline fits to the scaled proton collision strengths.
%file: si_7.psplups %rates: Ryans R.S.I., Keenan F.P., Reid R.H.G., unpublished. %energies: Observed values, from .elvlc file %comment: Fits valid for temperatures 1.75e5 to 6e6 K. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young 15-May-2001
Page created by Giulio Del Zanna on Wed Jun 8 16:14:32 2022