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- W1569135574 abstract "We present relative spectral line intensities for 16 3s-3p and 3p-3d transitions in the neonlike ion ${mathrm{Fe}}^{16+}$, obtained from solar-flare spectra. The spectra were obtained by a Naval Research Laboratory slitless spectrograph flown on the Skylab manned space station. The results are of relevance to x-ray-laser experiments involving collisional pumping of excited states of neonlike ions, and to the analysis of solar-flare spectra. The relative line intensities are measured to an accuracy of about 30%. The measured line intensities are compared with theoretical line intensities calculated assuming electron collisional excitation within the ${mathrm{Fe}}^{16+}$ ion followed by deexcitation and radiative decay. The measured and theoretical intensities agree to within less than a factor of 2 for all but one line. The important J=0 lines (3 $^{1}mathrm{S}_{0}$--3s $^{1}mathrm{P}_{1}$,3s $^{3}$${mathit{P}}_{1}$) at 254.87 and 204.65 AA{} are about a factor of 1.4 weaker than predicted, which is almost within experimental error. The 3${mathit{s}}^{3}$${mathit{P}}_{2}$--3p $^{3}$${mathit{S}}_{1}$ line at 409.69 AA{} is 2.3 times weaker than predicted, and this is unexplained." @default.
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- W1569135574 date "1991-03-01" @default.
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- W1569135574 title "Intensities of the neonlike iron (<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant=normal>Fe</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn><mml:mn>6</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math>) 2<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant=italic>p</mml:mi></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow></mml:…" @default.
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- W1569135574 doi "https://doi.org/10.1103/physreva.43.2565" @default.
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