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In 1995, when Earth passed through the ring plane, the edge-on viewing geometry permitted a direct determination of the ring thickness and a precise measurement of the rate of precession of Saturn's rotational axis.
No Continuousriginandty is madiscontinuous hoped that present results will be of interest to designers.
Then we introduce the bio-inspired particle swarm optimization (PSO) to study the ring thickness distribution.
The globally optimized ring thickness distribution providing the maximal mechanical sensitivity is obtained and detailedly discussed.
Based on this, we study how do basic structure parameters of the DRG affect the optimum ring thickness distribution.
We calculate the mechanical sensitivity of the DRG with some given ring thickness distributions by using finite element analysis (FEA).
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The number of rings and cavities between them is finite as it is the ring thicknesses.
Those orbital correlations and gossamer ring thicknesses that match the motions of the moons have convinced Galileo team members that the gossamer ring dust is indeed coming from these two moons.
The architecture of the developed PEDD device illustrated in Fig. 1 fulfills the above requirements: The optical pathlength through the solution (determined by the o-ring thickness) is merely 250 μm.
Results show how much the E-field is influenced by the ring tube thickness.
The 500 and 800 MHz antennas were used for the GPR survey, and the main purpose was to obtain the inner ring stone thickness of the arch.
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