Solar MgI lines Stark broadening (Dimitrijevic+, 1996)

Details Solar MgI lines Stark broadening (Dimitrijevic+, 1996) Solar MgI lines Stark broadening (Dimitrijevic+, 1996)

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41170127d&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/117/127. Originally published in: 1996A&AS..117..127D

Physics

Atomic Physics

Atomic Physics

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.
(3 data files).

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