For more than 40 years, most astrophysical observations and laboratory studies of two key soft X-ray diagnostic 2p-3d transitions, 3C and 3D, in Fe XVII ions found oscillator-strength ratios $f_{3C}/ f_{3D}$ disagreeing with theory. This discrepancy hampered the proposed plasma diagnostic utility based on the observed intensity ratios ever since. In previous laboratory measurements, the ratio was determined by scrutinizing the photon emission of an electron-impact excited plasma. First X-ray laser spectroscopy experiments at a free-electron laser (FEL) confirmed the discrepancy between experiments and theory independently of electron-excitation cross sections that could have falsified previous laboratory measurements. In this thesis, the 3C...
Deutsche Forschungsgemeinschaft (DFG) Project No. 266229290.We determined relative X-ray photon emis...
Highly charged iron (Fe<sup>16+</sup>, here referred to as Fe xvii) produces some of the brightest X...
Highly charged iron (Fe161, here referred to as Fe XVII) produces some of the brightest X-ray emissi...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft X-ray...
We measured the L-shell soft X-ray fluorescence of Fe XVII ions in an electron beam ion trap followi...
One of the most enduring and intensively studied problems of x-ray astronomy is the disagreement of ...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray...
One of the most enduring and intensively studied problems of X-ray astronomy is the disagreement of ...
One of the most enduring and intensively studied problems of X-ray astronomyis the disagreement of s...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray...
We measured the L-shell soft X-ray fluorescence of Fe XVII ions in an electron beam ion trap followi...
We determined relative X-ray photon emission cross sections in Fe XVII ions that were mono-energetic...
X-ray emission from neon-like Fe XVII has been measured with high-resolution spectrometers from labo...
Highly charged iron (Fe(16+), here referred to as Fe XVII) produces some of the brightest X-ray emis...
Deutsche Forschungsgemeinschaft (DFG) Project No. 266229290.We determined relative X-ray photon emis...
Highly charged iron (Fe<sup>16+</sup>, here referred to as Fe xvii) produces some of the brightest X...
Highly charged iron (Fe161, here referred to as Fe XVII) produces some of the brightest X-ray emissi...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft X-ray...
We measured the L-shell soft X-ray fluorescence of Fe XVII ions in an electron beam ion trap followi...
One of the most enduring and intensively studied problems of x-ray astronomy is the disagreement of ...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray...
One of the most enduring and intensively studied problems of X-ray astronomy is the disagreement of ...
One of the most enduring and intensively studied problems of X-ray astronomyis the disagreement of s...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray...
For more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray...
We measured the L-shell soft X-ray fluorescence of Fe XVII ions in an electron beam ion trap followi...
We determined relative X-ray photon emission cross sections in Fe XVII ions that were mono-energetic...
X-ray emission from neon-like Fe XVII has been measured with high-resolution spectrometers from labo...
Highly charged iron (Fe(16+), here referred to as Fe XVII) produces some of the brightest X-ray emis...
Deutsche Forschungsgemeinschaft (DFG) Project No. 266229290.We determined relative X-ray photon emis...
Highly charged iron (Fe<sup>16+</sup>, here referred to as Fe xvii) produces some of the brightest X...
Highly charged iron (Fe161, here referred to as Fe XVII) produces some of the brightest X-ray emissi...