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Observed enhancement of K-shell radiative recombination (RR) of bare uranium ions with cooling electrons is interpreted in terms of of distant transverse collisions in magnetized electron-cooler plasma described within the semiclassical geometrical model (SGM), which was recently proposed. The Monte Carlo simulations based on the proposed approach explains the enhancement measured in RR of U^{92+} ions with cooling electrons for the K-shell

Enhanced radiative recombination of U92+ions with cooling electrons for the K-shell

Enhanced radiative recombination of U⁹²⁺ions with cooling electrons for the K-shell