The Fe IX spectrum features two lines in the extreme ultraviolet whose ratio has been rated among the best density diagnostics in the solar spectrum. One line is an E1-allowed intercombination transition at 244.909 Å, the other an E1-forbidden M2 transition at 241.739 Å. Employing a medium and a high resolution spectrometer at the Livermore EBIT-I electron beam ion trap, we have observed the line pair in the laboratory for the first time. Using a CHIANTI model computation, the observed line ratio yields a value of the electron density that is compatible with typical densities in our device
We report high-resolution density dependent intensity ratio measurements for middle charge states of...
The EUV spectrum of $\ion{Fe}{vii}$ is reviewed, using new rates for electron impact excitation, a...
The coronal lines that are observable in the Hinode EUV Imaging Spectrometer (EIS) wavelengths are a...
A multitude of weaker Fe IX lines have been predicted in the vicinity of the strong 171 Å line that ...
Previously, large discrepancies have been found between theory and observation for Fe XV emission li...
We analyzed spectral data of Fe XXII and Ar XIV from laboratory sources in which the electron densit...
New calculations of radiative rates and electron impact excitation cross sections for Fe XI are used...
Extreme-ultraviolet spectra of intermediately ionized iron ions (Fe VI-Fe XIV) in the wavelength ran...
Extreme-ultraviolet spectra of intermediately ionized iron ions (Fe VI-Fe XIV) in the wavelength ran...
The intensity ratio of Fe XIV 264.765A/274.203A is useful to determine the electron density of solar...
The EUV spectrum of Fe is reviewed, using new rates for electron impact excitation, atomic structu...
We use recently calculated electron collisional data by [CITE] for $\ion{Fe}{xii}$ ($n=3$ configura...
Many intensity ratios involving Fe XII 3s23p3_3s3p4 and 3s23p3-3s23p23d transitions in the 186-383 A...
We report new observations of emission line intensity ratios of Fe XVII under controlled experimenta...
The EUV spectrum of $\ion{Fe}{viii}$ is reviewed, using new solar observations from the Hinode EUV...
We report high-resolution density dependent intensity ratio measurements for middle charge states of...
The EUV spectrum of $\ion{Fe}{vii}$ is reviewed, using new rates for electron impact excitation, a...
The coronal lines that are observable in the Hinode EUV Imaging Spectrometer (EIS) wavelengths are a...
A multitude of weaker Fe IX lines have been predicted in the vicinity of the strong 171 Å line that ...
Previously, large discrepancies have been found between theory and observation for Fe XV emission li...
We analyzed spectral data of Fe XXII and Ar XIV from laboratory sources in which the electron densit...
New calculations of radiative rates and electron impact excitation cross sections for Fe XI are used...
Extreme-ultraviolet spectra of intermediately ionized iron ions (Fe VI-Fe XIV) in the wavelength ran...
Extreme-ultraviolet spectra of intermediately ionized iron ions (Fe VI-Fe XIV) in the wavelength ran...
The intensity ratio of Fe XIV 264.765A/274.203A is useful to determine the electron density of solar...
The EUV spectrum of Fe is reviewed, using new rates for electron impact excitation, atomic structu...
We use recently calculated electron collisional data by [CITE] for $\ion{Fe}{xii}$ ($n=3$ configura...
Many intensity ratios involving Fe XII 3s23p3_3s3p4 and 3s23p3-3s23p23d transitions in the 186-383 A...
We report new observations of emission line intensity ratios of Fe XVII under controlled experimenta...
The EUV spectrum of $\ion{Fe}{viii}$ is reviewed, using new solar observations from the Hinode EUV...
We report high-resolution density dependent intensity ratio measurements for middle charge states of...
The EUV spectrum of $\ion{Fe}{vii}$ is reviewed, using new rates for electron impact excitation, a...
The coronal lines that are observable in the Hinode EUV Imaging Spectrometer (EIS) wavelengths are a...