The K x-ray emission spectra of 3d transition elements have been with great interests for a long time because of their asymmetric shapes or the existence of satellite lines. These features indicate that some processes or interactions play an important role besides single electron transition between the levels of the diagram lines. Although multielectron excitations or multiplet splitting, etc. may be considered as origins of satellite lines, the origins of many satellite lines remain not clarified. Therefore, in order to elucidate the mechanism of their origins (especially of Kb ' and Kb " satellite lines) the K x-ray emission spectra of chromium in Cr metal, Cr2O3, CoCr2O4, FeCr2O4, K2CrO4 and K2Cr2O7 were measured using a double...
The Kß emission spectra of calcium, titanium, chromium, manganese and iron and oxidic compounds of t...
Les spectres de rayons X Kα du molybdène (Z=42), palladium (Z=46) et holmium (Z=67) bombardés par de...
We report on the global distribution of the intensities of the K-shell lines from He-like and H-like...
International audienceOne of the remarkable features of the X‐ray emission from the Galactic center ...
The financial support of the Swiss National Science Foundation (Grant No. 200020-146739) is acknowle...
Cet article traite de la modification du profil de raie (en particulier en ce qui concerne la largeu...
International audienceWe report on measurements of the K diagram, valence-to-core (VtC), and hypersa...
We analyze the core and valence transitions in chromium in a series of materials with a number of di...
International audienceThis article presents detailed experimental and theoretical studies of the sat...
All data tables associated with the article: 'Heterogeneous kimberlite metasomatism revealed from a ...
The multiplet structure of core-electron binding energies in Cr 3s, Cr 3p and Cr 2p levels of CrCl3 ...
This study focus on High Energy K X-ray satellites which are a particular category of characteristic...
The K-shell emission line of neutral iron from the Galactic center (GC) region is one of the keys co...
Satellite lines in the emission spectra of compounds are explained by assuming cross transitions; th...
We analyze the core and valence transitions in chromium in a series of materials with a number of di...
The Kß emission spectra of calcium, titanium, chromium, manganese and iron and oxidic compounds of t...
Les spectres de rayons X Kα du molybdène (Z=42), palladium (Z=46) et holmium (Z=67) bombardés par de...
We report on the global distribution of the intensities of the K-shell lines from He-like and H-like...
International audienceOne of the remarkable features of the X‐ray emission from the Galactic center ...
The financial support of the Swiss National Science Foundation (Grant No. 200020-146739) is acknowle...
Cet article traite de la modification du profil de raie (en particulier en ce qui concerne la largeu...
International audienceWe report on measurements of the K diagram, valence-to-core (VtC), and hypersa...
We analyze the core and valence transitions in chromium in a series of materials with a number of di...
International audienceThis article presents detailed experimental and theoretical studies of the sat...
All data tables associated with the article: 'Heterogeneous kimberlite metasomatism revealed from a ...
The multiplet structure of core-electron binding energies in Cr 3s, Cr 3p and Cr 2p levels of CrCl3 ...
This study focus on High Energy K X-ray satellites which are a particular category of characteristic...
The K-shell emission line of neutral iron from the Galactic center (GC) region is one of the keys co...
Satellite lines in the emission spectra of compounds are explained by assuming cross transitions; th...
We analyze the core and valence transitions in chromium in a series of materials with a number of di...
The Kß emission spectra of calcium, titanium, chromium, manganese and iron and oxidic compounds of t...
Les spectres de rayons X Kα du molybdène (Z=42), palladium (Z=46) et holmium (Z=67) bombardés par de...
We report on the global distribution of the intensities of the K-shell lines from He-like and H-like...