C. Senemaud Created 2026-10-18 Updated 2026-11-05
A contributor to international nomenclature recommendations for X-ray spectroscopy. The system relates line names to electronic energy levels instead of requiring a separate historical label for every transition, making complicated spectra easier to describe consistently.[ref]
R. Jenkins Created 2026-10-18 Updated 2026-11-05
A scientific contributor to IUPAC recommendations that standardize names for X-ray spectroscopy. The proposed notation identifies emission lines and absorption edges through their underlying energy-level designations, making the physical transition easier to compare across measurements and publications.[ref]
R. Manne Created 2026-10-18 Updated 2026-11-05
A contributor to a standardized notation for X-ray spectroscopy. Naming a line through the electronic levels involved reduces reliance on historical labels. The resulting nomenclature gives experimentalists a consistent way to communicate which atomic transition a measured feature represents.[ref]
R. Robin Created 2026-10-18 Updated 2026-11-05
A scientific contributor to IUPAC recommendations for labeling X-ray emission lines and absorption edges. Connecting a spectral label with an energy-level designation makes the notation applicable to different transitions, improving the comparability of spectroscopic descriptions.[ref]
X unit 2026-10-18
The historical X unit was a practical X-ray wavelength unit, approximately . Its scale used an assigned calcite spacing; relative wavelength measurements could be more precise than absolute determinations. Variation between crystal specimens led to calibration using reference spectral lines. An X unit value therefore cannot simply be read as an exact multiple of .[ref]
An angular-scale check determines how an indicated rotation corresponds to an angle. A reference line transfers a wavelength scale. An absolute determination ties that scale to an independently established length standard. These are different calibration tasks. Repeating measurements can reduce random scatter without correcting the common scale: if every inferred is too large by a chosen , all inferred absolute wavelengths are too large by , while ratios using that same are unchanged.