1930
DOI: 10.1007/bf02079933
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Zur Theorie der Elastizität flacher rotationssymmetrischer Schalen

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Cited by 9 publications
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“…This approach is usually referred to as 'asymptotic integration' in the thin-shell literature and it amounts to exploiting the presence of the ubiquitous parameter 0 < (h/R) 1 (see Figure 1) in order to derive WKB-type approximations for the corresponding thin-shell equations. Blumenthal [3,4], Geckler [27,28], and Hetényi [34] are some of the key names associated with fundamental developments in this area. The case of non-axisymmetric deformations in thin spherical shells was originally tackled by Havers [32] (see also Flügge's account in [24]), who also discovered that Blumenthal's earlier approach was still relevant to deformations lacking radial symmetry provided that some small mathematical adjustments were introduced.…”
Section: Introductionmentioning
confidence: 99%
“…This approach is usually referred to as 'asymptotic integration' in the thin-shell literature and it amounts to exploiting the presence of the ubiquitous parameter 0 < (h/R) 1 (see Figure 1) in order to derive WKB-type approximations for the corresponding thin-shell equations. Blumenthal [3,4], Geckler [27,28], and Hetényi [34] are some of the key names associated with fundamental developments in this area. The case of non-axisymmetric deformations in thin spherical shells was originally tackled by Havers [32] (see also Flügge's account in [24]), who also discovered that Blumenthal's earlier approach was still relevant to deformations lacking radial symmetry provided that some small mathematical adjustments were introduced.…”
Section: Introductionmentioning
confidence: 99%