Resonantly excited metal K core line spectra of NiO, MnO, CuO and other com
pounds have been investigated at the beamlines X21 (NSLS/BNL), BW1 and W1.1
(HASYLAB/DESY). A novel technique for quantitative resolution of NEXAFS sp
ectra into spin-up and spin-down components has been developed. Since the m
ethod employs spin conservation and local spin references, it needs no circ
ularly polarized radiation and no sample magnetization for taking both the
RXS and NEXAFS spectra. Hence antiferromagnetic and paramagnetic materials
can be investigated as well. By utilizing linear dichroism with angular-dep
endent measurements on single-crystal samples, additional resolution of NEX
AFS spectra is possible with respect to the orbital symmetry. Application o
f the method to paramagnetic MnO, for the first time, provides new and unam
biguous experimental results confirming modern (LSDA+U) calculations.