Kαhypersatellites of Zr

Abstract
The Kα hypersatellites Kα1h and Kα2h of zirconium were observed in a conventional x-ray spectrum analysis. The energy separation between the hypersatellites and their corresponding diagram lines were measured, and the intensity ratio I(Kα1h)I(Kα2h) was computed. The experimental values are in good agreement with the results of the most advanced calculations, except for the energy of the Kα2h where the measured value is some 15 eV higher than the theoretical prediction.