Stark shifts and transition probabilities in the Ne II spectrum

Details Stark shifts and transition probabilities in the Ne II spectrum Stark shifts and transition probabilities in the Ne II spectrum

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...382..359d&link_type=abstract

Astronomy and Astrophysics, v.382, p.359-367 (2002)

Astronomy and Astrophysics

Astrophysics

22

Atomic Data, Radiation Mechanisms: General, Methods: Laboratory

Scientific paper

Stark shifts (d) and transition probabilities of the spontaneous emission (Einstein's A values) of forty two singly charged neon (Ne Ii) ion spectral lines have been measured in a linear, low pressure, pulsed arc at 35 300 K electron temperature and 1.83 x 1023 m-3 electron density. Transition probabilities have been obtained using the relative line intensity ratio (RLIR) method. Stark shift values have also been calculated, using the semiclassical perturbation formalism (SCPF). The measured and calculated shift values and the measured A values have been compared to the existing data taken from available data sources.

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