Kαhypersatellites of Mo

The $K{\alpha }_1^h$ and the $K{\alpha }_2^h$ hypersatellites of molybdenum were observed in a conventional x-ray spectrum analysis. The energy separation between the hypersatellites and the corresponding characteristic lines were measured and found to be in good agreement with the results obtained from Hartree-Fock calculations. The relative intensity ratio $\frac{K{\alpha }_1^h}{K{\alpha }_2^h}$ was computed and compared with the results of intermediate-coupling calculations.