We have measured relative x-ray-production cross sections for Ca Kα satellite and hypersatellite transitions produced from 24.0- to 48.0-MeV oxygen bombardment of thick targets. All cross-section ratios as functions of projectile energy for initial defect configurations KᵏLˡ, where $k=1, 2$ and $l=0, 1, 2, 3, 4$, are in qualitative agreement with configuration-space binary-encounter-approximation predictions.
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Olsen et al. (1974) studied this question.
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