Sentence examples for field of the shell from inspiring English sources

The former enhances the anisotropy field of the shell region and the latter weakens intergranular exchange coupling.

The displacement field of the shell and the sound pressure of the fluid are expanded by Fourier series and Chebyshev orthogonal polynomials.

These vectors, evaluated in the near field of the shell wall at several distances form the input force for increasing time, give insight into the exchange of energy between the structure and the fluid as the various waves propagate through the system.

The influence of this two temperature field on the shell's stable shapes was predicted analytically, which thereafter is determined by finite element results.

The far field mobility of the shell for each propagating circumferential modenis calculated using a residue method.

The reversal field of the outer shell is larger than that of the core and consequently the latter coincides with the global particle coercivity.

Fibre optic controlled instrumentation and high speed photography provide a vital insight towards coupled flow-field behaviour of the shell structure.

This problem is of particular interest because the Cosserat solution can be compared with an exact solution and the influences of variable shell thickness and strong variations of the temperature field through the shell's thickness can be explored independently.

The results of these examples show that the Cosserat theory is accurate for moderately thick shells and moderately strong variation of the temperature field through the shell's thickness.

The covering-domain method, which transforms the calculation of the scattering sound field of a complicated-shaped close cavity to that of a series of simply regular-shaped close shells such as close spherical shell and infinite cylindrical shell, is applied to calculating the scattering sound field of the plate-ended cylindrical shell structure.

Here, we analyze snapshots from self-consistent 3D numerical dynamos to unravel the nature of field-flow interactions that induces stretching secular variation of the radial magnetic field at mid-depth of the shell.