Non-hydrogen-bonded isomers were photogenerztted by UV (lambda > 335 nm) irradiation of o-hydroxybenzaldehyde (salicylaldehyde) and o-hydroxyacetophenone monomers isolated in low-temperature Ar matrixes. These photoisomerizations were found to be photoreversible. Upon shorter wavelength (lambda > 235 nm or lambda > 270 nm) UV irradiation, the initial forms of the compounds (with intramolecular hydrogen bonds) were partially repopulated. The structures of the photogenerated non-hydrogen-bonded isomers of both compounds were positively identified by comparison of their IR spectra with the spectra theoretically calculated [at the DFT(B3LYP)/6-311++G(2d,p) level] for all possible non-hydrogen-bonded isomers of the studied compounds. The experimental IR spectra of the photoproclucts generated from o-hydroxybenzaldehyde and o-hydroxyacetophenone are very well reproduced only by the theoretical spectra predicted for the isomers with both OH and formyl (or acetyl) groups rotated by 180, with respect to the initial, most stable hydrogen-bonded conformer. Excellent agreement between experiment and theoretical prediction provides a basis for a very reliable identification of the photoproduced isomers of o-hydroxybenzaldehyde and o-hydroxyacetophenone.