We are continuing EBIT measurements of line lists in the EUV region for use as astrophysical diagnostics and have recently measured the same transitions in much denser plasma of the NSTX tokamak. This allows us to calibrate density-sensitive line ratios at their upper limits. We compare our observations at low and high density with calculations from the Flexible Atomic Code
The electron beam ion trap (EBIT) facility at the Lawrence Livermore National Laboratory is being us...
Theoretical electron density-sensitive line ratios $R_1 - R_6$ of Ar XIV soft X-ray emission lines a...
Spectral line shapes and intensities are used for obtaining information on the various regions of ma...
We analyzed spectral data of Fe XXII and Ar XIV from laboratory sources in which the electron densit...
High-resolution measurements of K-shell emission from O, F, and Ne have been performed at the ASDEX ...
One of the dominant forms of astronomical line emission in the 6 {angstrom} to 18 {angstrom} spectra...
We present a comprehensive wavelength survey of Fe L-shell X-ray lines between 7 and 11 {angstrom} m...
We are developing an experimental database of extreme ultraviolet spectra from highly charged ions u...
Recent ASCA spectra exhibit discrepancies with the relative line intensities of various Fe XXIII and...
Extreme ultraviolet (EUV) spectra emitted from aluminum in the 5-340 A wavelength range were observe...
The EUV spectrum of Fe is reviewed, using new rates for electron impact excitation, atomic structu...
7th International Conference On Atomic and Molecular Data and Their Applications - ICAMDATA-2010, 21...
Using the Electron Beam Ion Trap facility at Lawrence Livermore National Laboratory, we have measure...
The coronal lines that are observable in the Hinode EUV Imaging Spectrometer (EIS) wavelengths are a...
We have systematically observed extreme ultraviolet (EUV) spectra from highly charged ions of nine l...
The electron beam ion trap (EBIT) facility at the Lawrence Livermore National Laboratory is being us...
Theoretical electron density-sensitive line ratios $R_1 - R_6$ of Ar XIV soft X-ray emission lines a...
Spectral line shapes and intensities are used for obtaining information on the various regions of ma...
We analyzed spectral data of Fe XXII and Ar XIV from laboratory sources in which the electron densit...
High-resolution measurements of K-shell emission from O, F, and Ne have been performed at the ASDEX ...
One of the dominant forms of astronomical line emission in the 6 {angstrom} to 18 {angstrom} spectra...
We present a comprehensive wavelength survey of Fe L-shell X-ray lines between 7 and 11 {angstrom} m...
We are developing an experimental database of extreme ultraviolet spectra from highly charged ions u...
Recent ASCA spectra exhibit discrepancies with the relative line intensities of various Fe XXIII and...
Extreme ultraviolet (EUV) spectra emitted from aluminum in the 5-340 A wavelength range were observe...
The EUV spectrum of Fe is reviewed, using new rates for electron impact excitation, atomic structu...
7th International Conference On Atomic and Molecular Data and Their Applications - ICAMDATA-2010, 21...
Using the Electron Beam Ion Trap facility at Lawrence Livermore National Laboratory, we have measure...
The coronal lines that are observable in the Hinode EUV Imaging Spectrometer (EIS) wavelengths are a...
We have systematically observed extreme ultraviolet (EUV) spectra from highly charged ions of nine l...
The electron beam ion trap (EBIT) facility at the Lawrence Livermore National Laboratory is being us...
Theoretical electron density-sensitive line ratios $R_1 - R_6$ of Ar XIV soft X-ray emission lines a...
Spectral line shapes and intensities are used for obtaining information on the various regions of ma...