Volume 400, Number 3, March IV 2003
|Page(s)||1155 - 1159|
|Section||Atomic, molecular, and nuclear data|
|Published online||07 March 2003|
Stark broadening parameters in the S III spectrum
Faculty of Physics, University of Belgrade, 11001 Belgrade, POB 368, Serbia, Yugoslavia
2 Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Yugoslavia
3 Astronomical Observatory 11160 Belgrade, Volgina 7, Serbia, Yugoslavia e-mail: email@example.com
Corresponding author: A. Srećković, firstname.lastname@example.org
Accepted: 20 December 2002
Stark widths and shifts of astrophysically important 10 doubly ionized sulfur (S III) spectral lines (within the 3d–4p and 4s–4p transitions) have been measured in a SF6 plasma created in the linear, low-pressure, pulsed arc discharge at about 35 000 K electron temperature and about m-3 electron density. The widths and shifts have been calculated using the semiclassical perturbation formalism (SCPF) (taking into account the impurity of energy levels, i.e. that the atomic energy levels are expressed as a mix of different configurations due to the configuration interaction), modified semiempirical (SEM) approximation, simplified semiclassical theory (G) and its modification (GM) taking into account new energy level values. Calculations have been performed for electron temperatures between 10 000 K and 150 000 K for electrons, protons and helium ions as perturbers. The measured and calculated S III shifts present the first published data in this field.
Key words: plasmas / line: profiles / atomic data
© ESO, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.