The spectrum of eight-times ionized iron, Fe ix, was studied in the 110–200 Å region. A low inductance vacuum spark and a 3 m grazing incidence spectrograph were used for the excitation and recording of the spectrum. Previous analyses of Fe ix have been greatly extended and partly revised. The number of known lines in the 3p 53d–3p 54f and 3p 53d–3p 43d 2 transition arrays is extended to 25 and 81, respectively. Most of the identifications of the Fe ix lines from the 3p 53d–3p 43d 2 transition array in the solar spectrum have been confirmed and several new identifications are suggested
In the light of accurate structure and scattering calculations for $\ion{Fe}{xvii}$, we review the ...
Recent fully relativistic calculations of radiative rates and electron impact excitation cross secti...
Iron spectra have been recorded from plasmas created at three different laser plasma facilities: the...
New spectrograms of multiply ionized iron have been recorded and analyzed, targeting the Fe vii spec...
The distorted wave extension of the autostructure code has been used to calculate energy levels, rad...
New calculations of radiative rates and electron impact excitation cross sections for Fe XI are used...
The EUV spectrum of $\ion{Fe}{vii}$ is reviewed, using new rates for electron impact excitation, a...
The spectrum of neutral iron is critical to astrophysics, yet furnace laboratory experiments cannot ...
We report preliminary measurements of Fe III spectra in the 1150 to 2500 A wavelength interval. Spec...
The EUV spectrum of Fe is reviewed, using new rates for electron impact excitation, atomic structu...
X-ray emission from neon-like Fe XVII has been measured with high-resolution spectrometers from labo...
The study of astrophysical spectra is reliant on accurate atomic data, and there is a need for the a...
We present new large-scale R-matrix (up to n = 4) and distorted-wave (DW, up to n = 6) scattering ca...
The EUV spectrum of $\ion{Fe}{viii}$ is reviewed, using new solar observations from the Hinode EUV...
Wavelengths for emission lines arising from 3s23p5-3s3p6 and 3s23p5-3s23p43d transitions in Ni XII h...
In the light of accurate structure and scattering calculations for $\ion{Fe}{xvii}$, we review the ...
Recent fully relativistic calculations of radiative rates and electron impact excitation cross secti...
Iron spectra have been recorded from plasmas created at three different laser plasma facilities: the...
New spectrograms of multiply ionized iron have been recorded and analyzed, targeting the Fe vii spec...
The distorted wave extension of the autostructure code has been used to calculate energy levels, rad...
New calculations of radiative rates and electron impact excitation cross sections for Fe XI are used...
The EUV spectrum of $\ion{Fe}{vii}$ is reviewed, using new rates for electron impact excitation, a...
The spectrum of neutral iron is critical to astrophysics, yet furnace laboratory experiments cannot ...
We report preliminary measurements of Fe III spectra in the 1150 to 2500 A wavelength interval. Spec...
The EUV spectrum of Fe is reviewed, using new rates for electron impact excitation, atomic structu...
X-ray emission from neon-like Fe XVII has been measured with high-resolution spectrometers from labo...
The study of astrophysical spectra is reliant on accurate atomic data, and there is a need for the a...
We present new large-scale R-matrix (up to n = 4) and distorted-wave (DW, up to n = 6) scattering ca...
The EUV spectrum of $\ion{Fe}{viii}$ is reviewed, using new solar observations from the Hinode EUV...
Wavelengths for emission lines arising from 3s23p5-3s3p6 and 3s23p5-3s23p43d transitions in Ni XII h...
In the light of accurate structure and scattering calculations for $\ion{Fe}{xvii}$, we review the ...
Recent fully relativistic calculations of radiative rates and electron impact excitation cross secti...
Iron spectra have been recorded from plasmas created at three different laser plasma facilities: the...