We report theoretical and experimental results of a study of spontaneous oscillations occurring in a fully ionized current-carrying plasma column. The experiment is performed in a linear discharge tube with annular electrodes that produces a plasma having large radial gradients of current density and resistivity. Under certain conditions it is found that the transverse magnetic field breaks into largeamplitude oscillations with a fairly well-defined frequency. 1 These oscillations are reminiscent of those occurring in the positive column under a sufficiently strong longitudinal magnetic field. 2 The degree of ionization in the positive column is, however, very low, and the theory of Kadomtsev and Nedospasov 3 which first successively explained those oscillations is based on assumptions that are not directly applicable to our case. On the other hand, most studies of highly conducting, current-carrying plasma using hydromagnetic equations including finite conductivity do not appear to have exhibited overstable modes. In particular, Kadomtsev 4 and, later, Furth, Killeen, and Rosenbluth 5 used such equations in a slab geometry and indeed found resistive instabilities, but they were all purely growing rather than oscillating. Moreover, Furth, Killeen, and Rosenbluth 5 Proc. Natl. Acad. Sci. IL S 0 57, 1164 (1967); and further literature cited therein. 5 The pressure spectrum function is defined in G. K. Batchelor, The Theory of Homogeneous Turbulence (Cambridge University Press, New York, 1953), p. 179. The pressure spectrum ir(k) is proportional to Ai(k) and Batchelor has shown that subject to a Gaussian velocity distribution of the velocities of an isotropic turbulent fluid 7T(k) = (1/8TT 2 )/£ (V )E (|k-k' |)(sin 4 0/ lk-k' l 4 )dk', £•"£' -W cos0, with E(k)dk the contribution to kinetic energy from wave numbers whose magnitudes lie between k and k + dk. exhibited a quadratic form from which they deduced quite generally that no overstable modes would exist in an incompressible plane-stratified plasma. Woods 6 extended Kadomtsev's analysis to a cylindrical plasma and reconfirmed the latter's original conclusion that, while a conductivity gradient in a current-carrying plasma can reduce the damping of Alfv£n waves, it will not lead to growth (overstability) at frequencies below the ion-cyclotron frequency. The analysis of Furth, Killeen, and Rosenbluth 5 was also extended to Stellarator geometries by Johnson, Greene, and Coppi, 7 and to cylindrical geometries by Coppi, Greene, and Johnson, 8 but these authors restricted their attention to the purely growing modes that are driven by a pressure gradient in a plasma of uniform resistivity. It should be added that an overstable mode was found by Jukes 9 in an analysis of a rather specialized model consisting of an annular current sheet separating an unionized core from a vacuum region.In those models which include a resistivity gradient 5 ? 8 the absence of overstable modes appears to be a direct consequence of the incompressibility assumption. In fact, by dropping th...