The OIV 1407.3\AA /1401.1\AA\ emission-line ratio in a plasma

التفاصيل البيبلوغرافية
العنوان: The OIV 1407.3\AA /1401.1\AA\ emission-line ratio in a plasma
المؤلفون: Nessib, Nabil Ben, Alonizan, Norah, Qindeel, Rabia, Sahal-Bréchot, Sylvie, Dimitrijević, Milan S.
سنة النشر: 2013
المجموعة: Astrophysics
Physics (Other)
مصطلحات موضوعية: Astrophysics - Solar and Stellar Astrophysics, Physics - Atomic Physics
الوصف: Line ratio of O IV 1407.3 \AA/1401.1 \AA\- 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 $10^{8}$ cm$^{-3}$ to $10^{13}$ cm$^{-3}$ and for a fixed temperature of 50 000 K.
Comment: 6 pages, 1 figure, 2 tables. Accepted for publication in Advances in Space Research
نوع الوثيقة: Working Paper
DOI: 10.1016/j.asr.2013.10.021
URL الوصول: http://arxiv.org/abs/1311.1054
رقم الأكسشن: edsarx.1311.1054
قاعدة البيانات: arXiv
الوصف
DOI:10.1016/j.asr.2013.10.021