Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phys...43..147k&link_type=abstract
Physica Scripta (ISSN 0031-8949), vol. 43, Feb. 1991, p. 147-149.
Astronomy and Astrophysics
Astrophysics
1
Electron Density (Concentration), Emission Spectra, High Temperature Plasmas, Metallic Plasmas, Plasma Spectra, Titanium, Cosmic Plasma, Forbidden Transitions, Isoelectronic Sequence, Line Spectra
Scientific paper
Recent R-matrix calculations of electron excitation rates for transitions in Ti XIV are used to derive two different theoretical emission-line ratios as a function of the electron density values from 10 to the 10 to 10 to the 14/cu cm. The density values are applicable to astrophysical and tokamak plasmas. The results are found to be significantly different from those deduced if the distorted-wave electron rates of Bhatia et al. (1985) are adopted in the calculations. The results also lead to electron density estimates between a factor of 1.6 larger and 30 percent smaller for electron temperatures in the 1.5-6 x 10 to the 6 K range.
Baluja K. L.
Hibbert Alan
Keenan Francis P.
Mohan Man
Reid H. G. R.
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