Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1764690 | Advances in Space Research | 2014 | 5 Pages |
Abstract
Line ratio of O IV 1407.3 Å/1401.1 Å is calculated using mostly our own atomic and collisional data.Energy levels and oscillator strengths needed for this calculation have been calculated using a Hartree–Fock relativistic (HFR) approach. The electron collision strengths introduced in the statistic equilibrium equations are fitted by polynomials for different energies. Comparison has also been made with available theoretical results.The provided line ratio has been obtained for a set of electron densities from 108108 cm−3 to 10131013 cm−3 and for a fixed temperature of 50,000 K.
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Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Nabil Ben Nessib, Norah Alonizan, Rabia Qindeel, Sylvie Sahal-Bréchot, Milan S. Dimitrijević,