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Energy levels, radiative rates and electron impact excitation rates for transitions in Si III
Aggarwal, K. M.
2017, Atomic Data and Nuclear Data Tables, 117, 320-424
ABSTRACT: Energy levels and radiative rates (A-values) for four types of transitions (E1, E2, M1, and M2)
are reported for an astrophysically important Mg-like ion Si III, whose emission lines have been observed in
a variety of plasmas. For the calculations, well-known and widely-used GRASP code has been adopted, and
results are listed for transitions among the 141 levels of the 3 l 3l' and 3 l 4 l configurations. Experimental
energies are available for only the lowest 58 levels but there is no major discrepancy with theoretical
results. Similarly, the A-values and lifetimes show a satisfactory agreement with other available results,
particularly for strong E1 transitions. Collision strengths are also calculated, with the DARC code, and listed
for resonance transitions over a wide energy range, up to 30 Ryd. No similar results are available in the
literature for comparisons. However, comparisons are made with the more important parameter, effective
collision strength (Upsilon), for which recent R-matrix results are available for a wide range of transitions,
and over a large range of temperatures. To determine Upsilon, resonances have been resolved in a narrow
energy mesh, although these are not observed to be as important as for other ions. Unfortunately, large
discrepancies in Upsilon values are noted for about half the transitions. The differences increase with
increasing temperature and worsen as the upper level J increases. In most cases the earlier results are
overestimated, by up to (almost) two orders of magnitude, and this conclusion is consistent with the one
observed earlier for Be-like ions.
{
"status": "new",
"changetime": "2019-02-04T13:02:49Z",
"_ts": "1549285369825011",
"description": "{{{\nEnergy levels, radiative rates and electron impact excitation rates for transitions in Si III \nAggarwal, K. M.\n2017, Atomic Data and Nuclear Data Tables, 117, 320-424\n\nABSTRACT: Energy levels and radiative rates (A-values) for four types of transitions (E1, E2, M1, and M2) \nare reported for an astrophysically important Mg-like ion Si III, whose emission lines have been observed in \na variety of plasmas. For the calculations, well-known and widely-used GRASP code has been adopted, and \nresults are listed for transitions among the 141 levels of the 3 l 3l' and 3 l 4 l configurations. Experimental \nenergies are available for only the lowest 58 levels but there is no major discrepancy with theoretical \nresults. Similarly, the A-values and lifetimes show a satisfactory agreement with other available results, \nparticularly for strong E1 transitions. Collision strengths are also calculated, with the DARC code, and listed \nfor resonance transitions over a wide energy range, up to 30 Ryd. No similar results are available in the \nliterature for comparisons. However, comparisons are made with the more important parameter, effective \ncollision strength (Upsilon), for which recent R-matrix results are available for a wide range of transitions, \nand over a large range of temperatures. To determine Upsilon, resonances have been resolved in a narrow \nenergy mesh, although these are not observed to be as important as for other ions. Unfortunately, large \ndiscrepancies in Upsilon values are noted for about half the transitions. The differences increase with \nincreasing temperature and worsen as the upper level J increases. In most cases the earlier results are \noverestimated, by up to (almost) two orders of magnitude, and this conclusion is consistent with the one \nobserved earlier for Be-like ions.\n}}}",
"reporter": "gary",
"cc": "",
"resolution": "",
"time": "2017-09-20T18:26:23Z",
"component": "atomic/molecular data base",
"summary": "Si III atomic data",
"priority": "good to do",
"keywords": "",
"version": "",
"milestone": "no milestone",
"owner": "nobody",
"type": "enhancement"
}
The text was updated successfully, but these errors were encountered:
reported by: @CloudyLex
Migrated from https://www.nublado.org/ticket/402
The text was updated successfully, but these errors were encountered: