Evolution of the air-cavity during a depressurized Wave Impact. Part II: the dynamical field
PHYSICS OF FLUIDS
Autore/i: Lugni, C; Brocchini, Maurizio; Faltinsen, Om
Editore: American Institute of Physics:2 Huntington Quadrangle, Suite 1NO1:Melville, NY 11747:(800)344-6902, (631)576-2287, EMAIL: subs@aip.org, INTERNET: http://www.aip.org, Fax: (516)349-9704
Classificazione: 1 Contributo su Rivista
Abstract: The present paper on wave-impact events in depressurized environments completes the analysis of
Part I by focusing on the dynamical features of the impacts and on the influence of the ambient
pressure. Connection is made between the impact regimes typically described in the literature and
the stages described in Part I C. Lugni, M. Miozzi, M. Brocchini, and O. M. Faltinsen, “Evolution
of the air cavity during a depressurized wave impact. I. The kinematic flow field,” Phys. Fluids 22,
056101 2010. The stages of isotropic/anisotropic compression and expansion of the air cavity are
of particular interest. The impact duration at the wall is almost independent of its height above the
undisturbed surface level, but its intensity rapidly decreases in the body of the fluid the peak
pressure halves within the first two compression/expansion cycles. The time evolution of the
pressure loads on the wall is analyzed by means of the Hilbert transform and an empirical mode
decomposition of the signals. This enables identification of the intrinsic mode functions which best
fit the original signal during its evolution and quantification of the frequency downshifting which
characterize the whole process. The pressure decay, largely governed by air leakage out of the
cavity, is found to be very intense during the air cavity closure and the isotropic compression/
expansion cycle stages 1 and 2; the decay observed during stage 3, i.e., during the anisotropic
compression/expansion cycles, is weaker and independent of the vertical location down the wall.
Differences between the observed decay rates and those of a three-dimensional bubble in an infinite
fluid are mainly due to the bubble being two-dimensional, being close to the free surface and loosing
air. The role of both ullage and vapor pressures on the impact is described, respectively, by means
of the Euler and cavitation numbers. The frequency of the bubble oscillation depends on these
numbers in a way that is closely similar to that displayed by the bubble area
Scheda della pubblicazione: https://iris.univpm.it/handle/11566/31054