Recent gas puff experiments on the 7-MA Saturn machine identified a curved surface at the plasma-vacuum interface during the run-in phase of the implosion. Incorporating this topology into a corresponding two-dimensional magnetohydrodynamic calculation revealed that this curvature plays a surprisingly dominant role in mitigating Rayleigh-Taylor (RT) growth prior to stagnation. Calculations with both Saturn and representative PBFA-Z parameters show that sheath curvature contributes to the reduction in RT growth by convecting the instability to the edges of the pinch faster than it can grow.[S0031-9007 (97)03377-2] PACS numbers: 52.35.Py, 52.55.Ez, 52.65.KjTraditional Z-pinch implosions are known to be susceptible to the Rayleigh-Taylor (RT) instability [1,2], especially for thin foil loads [3]. To improve the implosion quality, gas puff loads with thicker shells were subsequently developed. However, experiments have never demonstrated acceptable radiation performance with large diameter, high-velocity annular implosions [3,4]. For example, Saturn [5] data with annular gas puffs have shown significant instability growth and poor radiation emission at diameters of 4.5 cm [6,7]. Many techniques have been suggested to reduce RT development in conventional loads without substantially degrading the compression ratio of the pinch. Such techniques include uniform fills [8,9], puff on puff [10-12], B z or shear stabilization [13][14][15], and tailored density profiles [16,17]. Uniform fills, in particular, have been investigated both experimentally and theoretically.In a recent set of experiments on the 8-MA Saturn generator, the effect of uniform fill loads on stability was examined using neon-argon and krypton-argon gas mixtures [18]. These experiments demonstrated an improvement in implosion quality compared to corresponding annular loads. In addition, a unique feature associated with the uniform-fill loads was identified. Based on images from a high resolution, space-and time-resolved pinhole camera, a curved sheath was clearly seen at the plasma-vacuum interface during the observable portion of the implosion phase. This "hourglassing" [19] effect is shown in the experimental pinhole camera images of Fig. 1 and is attributed to the divergence of the gas flow coupled with an axial mass gradient. This is similar to the long wavelength effects that produce zippering [20,21]. It is evident from the figure that the hourglassing is fairly severe, and is maintained throughout the implosion.The detection of hourglassing in this set of experiments has led to speculation concerning the role, if any, that sheath curvature may play in instability growth or reduction. To examine this issue, a number of 2-dimensional magnetohydrodynamic (MHD) calculations were performed using the MACH2 [22] code. In these calculations, the injected gas distribution was simulated by a uniform density, right circular cylinder, with a concave outer surface and height of 2.0 cm. Imposing the curved outer surface of the load as an initial condition prov...