Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....34..363s&link_type=abstract
Astronomy and Astrophysics, vol. 34, no. 3, Sept. 1974, p. 363-370. Deutsche Forschungsgemeinschaft
Astronomy and Astrophysics
Astrophysics
Argon, Plasma Heating, Thermodynamic Equilibrium, Transition Probabilities, Electron Density (Concentration), Error Analysis, Plasma Temperature, Temperature Distribution
Scientific paper
A plasma-oven is described which produces a stationary, homogeneous plasma in the astrophysically interesting temperature range from 3000 to 8000 K. With this plasma-oven, containing argon with small admixtures of hydrogen, Ar-I transition probabilities have been determined. The Ar-I transition probabilities show no detectable dependence on the electron density, suggesting that there are no noticeable departures from LTE. The results are compared with other experiments and a detailed discussion of the errors is given.
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