Results 11 to 20 of about 597,270 (283)
Stark broadening of Zn II spectral lines
Monthly Notices of the Royal Astronomical Society, 2021 Stark broadening parameters, full widths at half intensity maximum, and shifts for 34 multiplets of singly charged zinc ion have been calculated using the impact semiclassical perturbation formalism.
M. Dimitrijević +3 more
semanticscholar +3 more sources
Stark Broadening of N VI Spectral Lines
Universe, 2023 Stark broadening parameters, line widths and shifts, for 15 N VI multiplets are calculated using semiclassical perturbation theory for temperatures from 50,000 K to 2,000,000 K, and perturber density of 1016 cm−3. As perturbers have been taken electrons,
Milan S. Dimitrijević +2 more
doaj +5 more sources
Stark broadening parameter tables for Ar VIII [PDF]
Serbian Astronomical Journal, 1999 Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line widths and shifts for 9 Ar VIII transitions as a function of temperature and perturber density.
Dimitrijević M.S., Sahal−Bréchot S.
doaj +5 more sources
Stark Broadening from Impact Theory to Simulations
Atoms, 2017 Impact approximation is widely used for calculating Stark broadening in a plasma. We review its main features and different types of models that make use of it.
Milan Dimitrijevic +2 more
exaly +3 more sources
Stark Broadening of Several Ne II, Ne III and O III Spectral Lines for the Stark-B Database [PDF]
Open Astronomy, 2011 In order to complete Stark broadening data for Ne II and O III lines, needed for analysis of stellar atmospheres, we determined the missing parameters for the broadening by collisions with protons and ionized helium for 15 Ne II and 5 O III multiplets ...
Dimitrijević Milan S. +3 more
doaj +2 more sources
Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
Atoms, 2018 Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas.
Milan Dimitrijevic +2 more
exaly +3 more sources
Spectroscopic measurement of Stark broadening parameter of the 636.2 nm Zn I-line
Natural Science, 2013 In this article we will present an attempt to measure the Stark broadening parameter of the Zn I-line at 636.23 nm utilizing the optical emission spectroscopy (OES) technique, taking into consideration the possibility of existence of self absorption.
A. M. E. Sherbini +6 more
exaly +2 more sources
Interpretation of Stark broadening measurements on a spatially integrated plasma spectral line. [PDF]
European Physical Journal : Applied physics, 2022 In thermal plasma spectroscopy, Stark broadening measurement of hydrogen spectral lines is considered to be a good and reliable measurement for electron density.
Julien Thouin +3 more
semanticscholar +1 more source
On the stark broadening of Os II spectral lines [PDF]
Bulletin of Natural Sciences Research, 2020 Stark broadening parameters, full widths at half maximum (FWHM) and shifts for 13 Os II lines have been calculated. The plasma parameters are: electron density of 1017 cm-3 and temperatures from 5 000 K to 80 000 K.
Dimitrijević Milan S.
doaj +2 more sources
Data on Stark Broadening of N VI Spectral Lines
DataData on Stark broadening parameters, spectral line widths, and shifts for 15 multiplets of N VI, whose spectral lines are broadened by collisions with electrons, protons, alpha particles (He III) and B III, B IV, B V and B VI ions, are presented.
Milan S. Dimitrijević +2 more
doaj +2 more sources