Stark broadening of solar MG I lines.

Details Stark broadening of solar MG I lines. Stark broadening of solar MG I lines.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..117..127d&link_type=abstract

Astronomy and Astrophysics Supplement, v.117, p.127-129

Astronomy and Astrophysics

Astrophysics

12

Lines: Profile, Atomic And Molecular Data, Sun: Photosphere, Sun: Chromosphere

Scientific paper

Using a semiclassical approach, we have calculated electron-, proton-, Mg II-, Si II-, Fe II-, and Ar II- impact line widths and shifts for 267 Mg I multiplets, in order to provide the needed Stark broadening parameters for all important perturbers for investigation of Solar and laboratory plasma. An analysis of Solar Rydberg lines in the far infrared spectrum has been performed as well.

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