Small deflection of a class of clamped thin plates using collocation

Equations are given for the optimization of a class of two-and three-dimensional structures. The application of existing analytical techniques to the response of thin clamped plates is described. The ratios of deflections to plate thickness are given for uniform transverse loads as well as for uniform plus linearly varying transverse loads. Deflections are presented at angular increments of 5 degrees and at radial increments of 0.1 of the radius

Geometrical and inertial properties of a class of thin shells of a general type

IBM 7094 Fortran program for evaluating surface area, centroids of surface volume or masses, and moments of inertia for thin walled shell

Orbit selection study for pageos satellite final report

Orbit selection for PAGEOS geodetic satellit

The conformal mapping of the interior of the unit circle onto the interior of a class of smooth curves

Outer and inner curved plates and shell shapes optimized by conformal mappin

Tables of natural frequencies and nodes for transverse vibration of tapered beams

Natural frequencies, nodal points, and mode functions for transverse vibration of tapered beam

Ba & Eu Abundances in M15 giant stars

To investigate the Ba and Eu abundances for a sample of 63 giant stars in the globular cluster M15. This is the largest sample of M15 giants stars for which Ba abundances have been determined and, due to the target selection of the original research programme, the Ba abundances are complete along the red giant branch. Stellar parameters were taken from the previous key study and a microturbulence-surface gravity relation was determined for precise measurement of the Ba line at 6496.898 Angstroms, which has a high sensitivity to microturbulence. Element abundances for Ba, La, Eu, Ca, Ni and Fe were calculated using spectrum synthesis and equivalent widths techniques. A bimodal distribution in Ba, Eu and La abundances was found within the sample. The low Ba,Eu,La mode had mean abundances of =-2.41+/-0.16, =-1.80+/-0.08 and =-2.19+/-0.13 while the high Ba,Eu,La mode had mean abundances of =-2.00+/-0.16, =-1.65+/-0.13 and =-1.95+/-0.11. Both modes are indicative of a pollution scenario dominated by the r-process, hence contributions from explosive nucleosynthesis of massive stars. There may be evidence of further enhancement by another heavy element process and of potential anticorrelations in Na-O for both modes indicating a complex formation and evolution history for M15.Comment: 20 pages, 15 figure

A method for determining an optimum shape of a class of thin shells of revolution

Optimum shape of convex thin shell of revolution with respect to volume, weight and length - mathematical functio

METHODOLOGY FOR TREND ANALYSIS AND PROJECTION OF PRODUCTION, MARKET SHARES, AND CONSUMPTION

Food Consumption/Nutrition/Food Safety,