The problem of resonance short-wave vibrations of a closed ellipsoidal elastic shell of revolution in a fluid is examined. An asymptotic solution (with respect to a large frequency parameter) is constructed for the Helmholtz equation for the acoustic pressure mode matched to the solutions of the system of equations of relative shell displacement. Is is shown that the radiation of a vibrating shell is governed by the location of the transition surfaces (TS) in the fluid and the transition lines on the shell that separate the non-wave zone with intensive pressure damping in the neighbourhood of the shell from the remote slowly damping radiation field. Regularities are investigated for the motion of the TS as the vibration frequency, circumferential wave number, and degree of curvature (prolateness) of the shell change. Estimates are given of the applicability of the asymptotic approach. It is known that the vibrations of shells of revolution of non-constant curvature in a vacuum occur with the formation of transition lines in certain frequency bands, where the nature of the state of shell stress and strain changes /1/. It is natural to expact that this property is conserved even for shell vibrations in a fluid, where TS also originate in the fluid because of the connectedness between the shell and fluid vibration modes. Interest in studying TS in fluids gave rise to a tendency to construct a solution of the problem that is valid both in the fluid layer surrounding the shell and in the far field. If radiation is not taken into account, then a problem is obtained that is similar to problems on shell vibrations in an incompressible fluid, whose solution for the pressure in the medium does not change its nature with distance from the shell. This problem is solved effectively by approximate analytical methods (see /2/, say). However, such a problem leaves open questions about the amplitudes of the resonant vibrations modes of the “shell-fluid” system, their damping because of energy radiation, and on the radiation field itself. Knowledge of the location of the TS as the connecting link between the near and far pressure fields in the fluid is the key to the solution of these questions within the framework of approximate methods.
Read full abstract