Non-LTE profiles of strong solar lines

Details Non-LTE profiles of strong solar lines Non-LTE profiles of strong solar lines

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976conm....1..110s&link_type=abstract

In its Contrib. of the Observatory of N. Mex. State Univ., Vol. 1, No. 4, p 110-122 (SEE N76-29085 19-89)

Computer Science

Atmospheric Models, Line Spectra, Solar Atmosphere, Calcium, Linearization, Magnesium, Sodium, Temperature Profiles, Transition Temperature, Turbulence

Scientific paper

The complete linearization method is applied to the formation of strong
lines in the solar atmosphere. Transitions in Na(I), Mg(I), Ca(I),
Mg(II), and Ca(II) are computed with a standard atmosphere and
microturbulent velocity model. The computed profiles are compared to
observations at disk center.

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