Mathematics
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...75...47h&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 75, no. 1, Oct. 1988, p. 47-51. Research sponsored by Polska
Mathematics
6
Metallic Plasmas, Partitions (Mathematics), Titanium, Vanadium, Atoms, Functions (Mathematics), Ionization, Particle Energy
Scientific paper
More realistic numerical values of the atomic partition functions U(r) for Ti-I, Ti-II, Ti-III, V-I, V-II, and V-III are given. The U(r) values are calculated in the temperature range of 2000-40,000 K, for the lowering of the ionization energy in the range of E(r) from 0.01 eV to 2 eV. The E(r) range from 0.1 to 0.01 corresponds to standard physical conditions in stellar atmospheres and partially to laboratory arc plasma conditions.
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