X-RayL-Series Satellite Lines

A theoretical treatment is given of the $L\alpha$ and $L\beta$ x-ray satellite lines. The satellites are assumed to arise from doubly-ionized atoms, and calculations of wave-length positions and of relative intensities are made on the method of the self-consistent field. Comparison of computed and observed satellite profile structure is made. A classification of reported experimental component lines is proposed in terms of theoretical transitions.