Theoretical Stark broadening parameters of Pbv spectral lines
Monthly Notices of the Royal Astronomical Society, ISSN: 1365-2966, Vol: 427, Issue: 2, Page: 1312-1321
2012
- 5Citations
- 2Captures
Metric Options: CountsSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
In this paper, we report calculated values of the Stark widths and shifts for 72 spectral lines of Pb v. They were calculated using the Griem semi-empirical approach. A set of wavefunctions obtained from Hartree-Fock relativistic calculations including core polarization effects was used. Stark widths and shifts corresponding to lines arising from 5dns (n = 7, 8), 5d6p, 5d6d and 5d5f configurations of Pb v. Stark widths and shifts are presented for an electron density of 10cm and temperatures T = 1.6-5.0 (10K). The 2142.5, 2167.9 and 2278.6Å lines of Pb v recently measured are included in our calculations. In this case, we have included for comparison calculations without core polarization effects. There is good agreement between our calculations and the above-cited experimental values. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84869785175&origin=inward; http://dx.doi.org/10.1111/j.1365-2966.2012.22081.x; https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2012.22081.x; https://dx.doi.org/10.1111/j.1365-2966.2012.22081.x; https://academic.oup.com/mnras/article/427/2/1312/976022
Oxford University Press (OUP)
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know