Presented here are the results of a series of experiments which explore the dissociation patterns of the clusters [O-2.(H2O)(n)](+) and O-4(+). H2O, where n is in the range 1-5. These clusters have been studied in order to identify reaction channels which may convert O-2(+), as seen in the E-region of the ionosphere, into H+(H2O)(n) clusters, which are the dominant ions in the lower D-region. Each [O-2.(H2O)(n)](+) ion can be viewed as a half-collision intermediate in the sequence of bimolecular hydration reactions, which are thought to lead to the formation of proton hydrates. Three different methods of cluster dissociation have been investigated, unimolecular (metastable) decay, collision-induced fragmentation, and photodissociation by visible laser radiation (450-690 nm). The experiments show that the intermediates [O-2.(H2O)(n)](+), for n in the range 2-5, preferentially dissociate to form (H2O)(n)(+) ions, a route which is largely favored over proton hydrate formation. For the first member of the series, O-2(+). H2O both collisional activation and photoexcitation lead to the appearance of O-2(+) and H2O as the major fragments For the trimer, [O-2.(H2O)(2)](+), the principal photofragment is (H2O)(2)(+) but a significant fraction of H3O+ is also observed. Each of the photodissociation channels observed for O-2(+). H2O and [O-2.(H2O)(2)](+) exhibits a much wider wavelength dependency than has been observed in previous experiments (Smith, G. P.; Lee, L. C. J. Chem. Phys. 1978, 69, 5393. Beyer, R. A.; Vanderhoff, J. A. J. Chem. Phys. 1976, 65, 2313). However, we are able to reproduce these earlier measurements by monitoring the photodissociation of "cold" clusters in the form O-2(+). H2O . Ar and [O-2.(H2O)(2). Ar](+). A new photodissociation cross section of (9 +/- 2) x 10(-18) cm(2) has been determined for the reaction O-2(+). H2O + h upsilon --> O-2(+) + H2O in the wavelength range 450-690 nm. Taken in conjunction with the solar radiation flux at 87 km, the magnitude of the corresponding unimolecular rate constant (10.8 s(-1)) suggests that the above process in association with "warm" ions may provide an important sink, which could explain the low O-2(+). H2O ion concentration observed in the ionosphere (McCrumb, J. L. Planet. Space Sci. 1982, 30, 559). A new rate constant of 2.4 s(-1) has also been estimated for the photodissociation of "warm＇＇ [O-2.(H2O)(2)](+) in conjunction-with the solar radiation flux at 87 km.