Buckling of Spherical Shells
Buckling of Spherical Shells
Buckling of Spherical Shells
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theory and experiment. There was no reason to doubt the classical theory <strong>of</strong> elasticity, which<br />
worked well for flat plates, and it was soon suspected that the effect <strong>of</strong> curvature and spherical shape<br />
imperfections could have been responsible for the discrepancies.<br />
This thesis led to the realization that the classical theory must have failed to reveal the fact that<br />
for a vessel configuration, not far away but somewhat different from the perfect geometry, lower<br />
total potential energy was involved, and therefore a lower value <strong>of</strong> buckling load could be expected,<br />
such as that indicated by tests. The theoretical challenge then became to formulate a solution<br />
compatible with such a lower boundary <strong>of</strong> collapse pressure at which the spherical shell could<br />
undergo the ‘‘oil canning’’ or ‘‘Durchschlag’’ process.<br />
After making a number <strong>of</strong> necessary simplifying assumptions, von Kármán and Tsien [2]<br />
developed a formula for the lower elastic buckling limit for collapse pressure, which for n ¼ 0.3<br />
was found to be<br />
P CR ¼ 0:37E=m 2 (31:3)<br />
This level <strong>of</strong> collapse pressure may be said to correspond to the minimum theoretical load necessary<br />
to keep the buckled shape <strong>of</strong> the shell with finite deformations in equilibrium. The lower limit<br />
defined by Equation 31.3 appeared to compare favorably with experimental results, also given in<br />
the literature [2]. On the other hand, the upper buckling pressure given by Equation 31.1 could be<br />
approached only if extreme manufacturing and experimental precautions were taken. In practice, the<br />
buckling pressure is found to be closer to the value obtained from Equation 31.3 and therefore this<br />
formula is <strong>of</strong>ten recommended for design.<br />
The exact calculation <strong>of</strong> the load–deflection curve for a spherical segment subjected to uniform<br />
external pressure is known to involve nonlinear terms in the equations <strong>of</strong> equilibrium, which cause<br />
substantial mathematical difficulties [3].<br />
31.4 PLASTIC STRENGTH OF SPHERICAL SHELLS<br />
Equations 31.2 and 31.3 may be regarded as design formulas based upon results using elasticity<br />
theory. Bijlaard [4], Gerard [5], and Krenzke [6] conducted subsequent studies to determine<br />
the effect <strong>of</strong> including plasticity upon the classical linear theory. To this end, Krenzke [6] conducted<br />
a series <strong>of</strong> experiments on 26 hemispheres bounded by stiffened cylinders. The materials were<br />
6061-T6 and 7075-T6 aluminum alloys, and all the test pieces were machined with great care at the<br />
inside and outside contours. The junctions between the hemispherical shells and the cylindrical<br />
portions <strong>of</strong> the model provided good natural boundaries for the problem. The relevant physical<br />
properties for the study were obtained experimentally. The best correlation was arrived at with the<br />
aid <strong>of</strong> the following expression:<br />
P CR ¼ 0:84(E sE t ) 1=2<br />
m 2 (31:4)<br />
where E s and E t are the secant and tangent moduli, respectively, at the specific stress levels. These<br />
values can be determined from the experimental stress–strain curves in standard tension tests. The<br />
relevant test ratios <strong>of</strong> radius to thickness in Krenzke’s work varied between 10 and 100 with a<br />
Poisson’s ratio <strong>of</strong> 0.3. The correlation based on Equation 36.4 gave the agreement between<br />
experimental data and the predictions within þ2% and 12%.<br />
The extension <strong>of</strong> the Krenzke results to other hemispherical vessels should be qualified.<br />
Although his test models were prepared under controlled laboratory conditions, the following<br />
detrimental effects should be considered in a real environment:<br />
ß 2008 by Taylor & Francis Group, LLC.