NASA NTRS ยท 19740052475
Shell deformation studies using holographic interferometry
Abstract
The buckling of shallow spherical shells under pressure has been the subject of many theoretical and experimental papers. Experimental data above the theoretical buckling load of Huang have given rise to speculation that shallow shell theory may not adequately predict the stability of nonsymmetric modes in higher-rise shells which are normally classified as shallow by the Reissner criterion. This article considers holographic interferometry as a noncontact, high-resolution method of measuring prebuckling deformations. Prebuckling deformations of a lambda = 9, h/b = 0.038 shell are Fourier-analyzed. Buckling is found to occur in an N = 5 mode as predicted by Huang's theory. The N = 4 mode was unusually stable, suggesting that even at this low value of h/b, stabilizing effects may be at work.
Keep this discovery
Explore connections, maps & timelines
Parmerter, R. R.. 1974-01-01. Shell deformation studies using holographic interferometry. https://ntrs.nasa.gov/citations/19740052475
Cite the original work for its findings. Save a collection to share your selection of sources.