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9 - VENTILATED SUPERCAVITIES 209
For the non-dimensional pulsation w
k
, WOODS obtains the following theoretical
relation:
wp
k
k=-117.
(9.22)
which has to be compared to equation (9.21). The higher the order of the pulsating
regime, the smaller the relative difference.
Finally, several features of two-dimensional ventilated cavities are very similar to
the case of axisymmetric cavities such as those theoretically described by P
ARISHEV
(1978) (see § 9.3).
9.2. AXISYMMETRIC VENTILATED SUPERCAVITIES
9.2.1. DIFFERENT REGIMES OF VENTILATED CAVITIES
For axisymmetric ventilated supercavities in horizontal flows, two main problems
have to be considered, the mode of evacuation of air at the rear of the cavity and
the deformation of the cavity under gravity [S
EMENENKO 2001, SAVCHENKO 2001].
Three modes of air leakage have been observed:
® When the F
ROUDE number
Fr V gd=
•
and the relative cavity underpressure s
c
are large enough, i.e. for large velocities and short cavities, gravitational effects
are small and the cavity is axisymmetric. Its tail is filled with foam which is
periodically rejected in the form of toroidal vortices (§ 9.2.2).
® For moderate values of the F
ROUDE number and long enough cavities (i.e. small
enough values of s
c
), gravity is important. The tail end of the cavity has two
hollow vortex tubes by which air is evacuated into the wake (§ 9.2.4).
® The third regime of gas leakage corresponds to pulsating cavities. It occurs for
high values of the flowrate coefficient. The behavior of axisymmetric pulsating
cavities is close to the 2D case described in section 9.1. It depends upon the
parameter
ss
cv
/
which plays a role similar to
ss
ca
/
introduced in section 9.1.2.
C
AMPBELL et al. (1958) suggested from empirical considerations that gravitational
effects would be important if:
s
c
Fr < 1
(9.23)
Values of
s
c
Fr
lower than 1 lead to the second regime of gas leakage by hollow
vortex tubes.
A different criterion, obtained theoretically by B
UYVOL (1980), covers the experimental
data better:
s
c
Fr
32
2
15
/
.<
(9.24)
Effectively, gravity is negligible for
s
c
Fr
32
2
/
larger than 10.