Published 1998 | Version Published
Conference Paper Open

Computing Shock Waves in Cloud Cavitation

Abstract

This paper presents a numerical investigation of some of the phenomena involved in the nonlinear dynamics of a homogeneous bubbly mixture bounded by an oscillatory wall. This problem represents an idealization of the flow in a typical vibratory cavitation damage device. Results are presented showing that wave steepening and ultimately shock wave formation occur as the magnitude of the excitation increases. The propagation characteristics of the waves through the bubbly medium have also been studied. Strong pressure peaks of short duration, corresponding to the coherent collapse of the bubble clusters, are computed and accurately resolved, both in space and time. As the amplitude of the excitation is increased a series of period doubling bifurcations occurs. The nonlinear dynamics of the oscillating bubble cluster are observed to follow a subharmonic route to chaos.

Additional Information

This research was supported, in part, by the Office of Naval Research under grant number N00014-91-J-1295. The third author is also grateful for support from the European Space Agency.

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Identifiers

Eprint ID
195
Resolver ID
CaltechAUTHORS:CEBcav98

Funding

Office of Naval Research (ONR)
N00014-91-J-1295
European Space Agency (ESA)

Dates

Created
2004-11-29
Created from EPrint's datestamp field
Updated
2019-10-02
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