Stark line broadening of 3s–3p and 3p–3d transitions of doubly ionized C, N, O, F and Ne

Blagojević, B.; Popović, M. V.; Konjević, N.

doi:10.1016/s0022-4073(99)00190-9

Cited by 14 publications

(31 citation statements)

References 23 publications

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“…A4, page 4 of 6 of N IV ion for various electron temperatures and densities along with the experimental results (Blagojević et al 1999(Blagojević et al , 2000Wrubel et al 1996Wrubel et al , 1998. The previous theoretical calculations w c of Ralchenko et al 2001), the full quantum mechanical calculations w 2 and its simplified calculations w 1 of Elabidi et al (2008) are also listed in Tables 1 and 2.…”

Section: Numerical Results and Discussionmentioning

confidence: 99%

“…Principally, all the corresponding experimental results cited in the present work have been published by two groups. The first group (Blagojević et al 1999(Blagojević et al , 2000 used a low-pressure pulsed arc and the second group (Wrubel et al 1996(Wrubel et al , 1998) used a gas-liner pinch. The accuracy of the experimental line widths is generally given by Konjević et al (2002) except for the few cases where other references have been mentioned.…”

Section: Numerical Results and Discussionmentioning

confidence: 99%

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Relativistic quantum mechanical calculations of electron-impact broadening for spectral lines in Be-like ions

Duan

Bari

et al. 2012

A&A

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Aims. We present relativistic quantum mechanical calculations of electron-impact broadening of the singlet and triplet transition 2s3s ← 2s3p in four Be-like ions from N IV to Ne VII. Methods. In our theoretical calculations, the K-matrix and related symmetry information determined by the colliding systems are generated by the DARC codes. Results. A careful comparison between our calculations and experimental results shows good agreement. Our calculated widths of spectral lines also agree with earlier theoretical results. Our investigations provide new methods of calculating electron-impact broadening parameters for plasma diagnostics.

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Section: Numerical Results and Discussionmentioning

confidence: 99%

Section: Numerical Results and Discussionmentioning

confidence: 99%

Relativistic quantum mechanical calculations of electron-impact broadening for spectral lines in Be-like ions

Duan

Bari

et al. 2012

A&A

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“…From the first experimental measurement of displacements of O III lines (Pretty 1931), Stark broadening parameters of O III lines have been measured several times (Platiša et al 1975;Purić et al 1988a,b;Blagojević et al 2000). Theoretically, Stark broadening of O III lines has been investigated by Subrahmaniam (1968), Hey & Bryan (1977), Dimitrijević & Konjević (1980, 1981, 1987, Hey & Breger (1980, 1981 and Dimitrijević (1981Dimitrijević ( , 1988a.…”

Section: Introductionmentioning

confidence: 99%

Stark broadening in O III spectrum

Srećković

Dimitrijević

Djeniže

2001

A&A

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Abstract. The Stark widths and shifts of 7 doubly ionized oxygen (O III) spectral lines, in five multiplets, have been measured at electron densities between 1.66 10 23 m −3 and 2.80 10 23 m −3 and electron temperatures between 17 000 K and 54 000 K in a linear pulsed-arc discharge in N2+ O2 and CO2 plasmas. The above mentioned species have been calculated using the semiclassical perturbation formalism. Our measured and calculated Stark width and shift values have been compared to the existing calculated and experimental data.

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“…2) are taken from Konjević & Pittman (1987), Purić et al (1988), Uzelac et al (1993), Blagojević et al (2000) and Milosavljević et al (2001). Here one should notice that the 2d level does not exist for Ne III.…”

Section: Analysis Of the Stark Halfwidths For The (N − 1)d -Np And Nsmentioning

confidence: 99%

“…Owing to these similarities, a gradual increase of the spectral line halfwidths, i.e., the systematic trend should be expected in these cases. For the analysis of (n − 1)d − np and ns−np transitions, the following references are available: Platiša et al (1975), Konjević & Pittman (1987), Purić et al (1988), Kobilarov & Konjević (1990), Uzelac et al (1993), Djeniže et al (1996), Iriarte et al (1997), Romeo y Bidegain et al (1998), Ahmad et al (1998), Blagojević et al (2000), Milosavljević et al (2000Milosavljević et al ( , 2001, Seidel et al (2001), Peláez et al (2006), Bukvić et al (2008), Peláez et al (2009Peláez et al ( ),Ćirišan et al (2011 and Djurović et al (2011).…”

Section: Introductionmentioning

confidence: 99%

Stark halfwidth trends along the homologous sequence of doubly ionized noble gases

Peláez

Djurović

Cirisan

et al. 2012

A&A

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Aims. The aim of this work is to analyze the behavior of experimentally determined Stark halfwidths for (n− 1)d− np and ns − np transitions along the homologous sequence of doubly ionized noble gases. Methods. We analyzed the Stark halfwidth trends including all available experimental data. Stark halfwidth results for the above mentioned transitions and corresponding multiplets were compared with the halfwidths calculated using the modified semiempirical formula (MSE) and the simplified modified semiempirical formula (SMSE). In case of Ne III the calculation made by semiclassicalperturbation formalism (SCPF) is also presented. Results. Stark halfwidths corresponding to (n − 1)d − np and ns − np transitions have been analyzed along the homologous sequence of doubly ionized noble gases. For all multiplets observed in this work, the analysis shows that the halfwidths of the spectral lines belonging to the same transition show a similar trend along the homologous sequence. Stark halfwidths of ns − np transitions have a clearly increasing trend. On the other hand, for (n − 1)d − np transitions, there are not enough data to make a similar conclusion. This type of trend analysis can be useful for Stark halfwidth predictions and hence for spectroscopic diagnostics of astrophysical plasmas.

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Stark line broadening of 3s–3p and 3p–3d transitions of doubly ionized C, N, O, F and Ne

Cited by 14 publications

References 23 publications

Relativistic quantum mechanical calculations of electron-impact broadening for spectral lines in Be-like ions

Relativistic quantum mechanical calculations of electron-impact broadening for spectral lines in Be-like ions

Stark broadening in O III spectrum

Stark halfwidth trends along the homologous sequence of doubly ionized noble gases

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