Stark broadening of the singly ionized xenon line - Temperature variation

Details Stark broadening of the singly ionized xenon line - Temperature variation Stark broadening of the singly ionized xenon line - Temperature variation

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrva..38.5742m&link_type=abstract

Physical Review A - General Physics, 3rd Series (ISSN 0556-2791), vol. 38, Dec. 1, 1988, p. 5742-5744.

Astronomy and Astrophysics

Astrophysics

14

Electron Plasma, Ionized Gases, Spectral Line Width, Stark Effect, Temperature Distribution, Xenon, Astrophysics, Electron Density (Concentration), Semiempirical Equations, Shock Tubes

Scientific paper

Linewidths of the 5419-A line are measured in a conventional shock tube. The Stark effect is the dominant broadening mechanism. Electron densities vary through the range 2.8 x 10 to the 16th - 2.2 x 10 to the 17th /cu cm, and temperatures vary from 8300 to 16,000 K. The Stark parameter increases by a factor of 2 as the temperature decreases. Results are compared with previous experimental data and semiempirical calculations.

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