Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199...37b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 199, Apr. 1982, p. 37-42.
Astronomy and Astrophysics
Astronomy
18
Abundance, Electron Oscillations, Line Spectra, Solar Atmosphere, Solar Spectra, Titanium, Accuracy, Atmospheric Models, Atomic Energy Levels, Atomic Excitations, Turbulence Effects
Scientific paper
An analysis is made of the seven most suitable 0 eV Ti I lines in the spectrum of the centre of the solar disc, using oscillator strengths of 0.5 per cent relative accuracy, and the solar model atmospheres of Holweger & Müller, and Vernazza et al. The solar abundance of titanium is found to be log A = 5.08 and the microturbulence is 1.00 km s-1, using the preferred atmosphere of Holweger & Müller.
Blackwell D. E.
Shallis M. J.
Simmons Guslavus J.
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