We report on a new technique, spin-polarized electron emission spectroscopy. Using grazing-angle, surface scattering of H⁺ and He⁺ ions at Ni(110), we find that the angle-resolved energy distribution of emitted spin-polarized electrons is significantly different from that of electron-induced secondary (cascade) electrons and exhibits a series of characteristic ``peaks'' (including element-specific Auger electrons). We obtain characteristic, spin-dependent information on the surface electronic structure of Ni(110) and on atom-surface charge-transfer processes.
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Rau et al. (1990) studied this question.
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