Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...434..779d&link_type=abstract
Astronomy and Astrophysics, Volume 434, Issue 2, May I 2005, pp.779-784
Astronomy and Astrophysics
Astrophysics
11
Sun: Atmosphere, Atomic Processes, Line: Formation, Polarization, Atomic Data
Scientific paper
We have developed a new semi-classical method for calculating the depolarization and polarization transfer rates of spectral lines of neutral and ionised atoms by collisions with atomic hydrogen (Derouich et al. 2003a, A&A, 404, 763; 2003b, A&A, 409, 369;
2004a, A&A, 414, 369; 2004b, A&A, 426, 707).
Up to now, our depolarization
rate calculations have been limited to simple atoms. In the present paper, we extend our theory to more complex atoms and we apply our new results to provide the first calculations associated
with the upper levels of multiplet 145 of neutral titanium Ti I which constitutes a remarkable example of the second solar spectrum (Manso Sainz & Landi Degl'Innocenti 2002, A&A, 394, 1093).
Barklem Paul S.
Derouich M.
Sahal-Bréchot Sylvie
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