Ag. Calamai et al., TRANSITION-PROBABILITIES FOR THE 3S(2)3P(P-2(0))-3S3P(2)(P-4) INTERSYSTEM LINES OF SI-II, The Astrophysical journal, 415(1), 1993, pp. 120000059-120000062
Intensity ratios of lines of the spin-changing ''intersystem'' multipl
et of Si II (4P --> 2P(o)) at 234 nm have been used to determine elect
ron densities and temperatures in a variety of astrophysical environme
nts. However, the accuracy of these diagnostic calculations have been
limited by uncertainties associated with the available atomic data. We
report the first laboratory measurement, using an ion-trapping techni
que, of the radiative lifetimes of the three metastable levels of the
3s3p2 4P term of Si II. Our results are 104 +/- 16, 406 +/- 33, and 81
1 +/- 77 mus for lifetimes of the J = 1/2, 5/2, and 3/2 levels, respec
tively. A-values were derived from our life-times by use of measured b
ranching fractions. Our A-values, which differ from calculated values
by 30% or more, should give better agreement between modeled and obser
ved Si II line ratios.