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The positional stability lines of a bubble in a bimodal driving field depends on
the amplitude of the second added frequency.
FIGs. 3 show the results of the sum
of forces on a
bubble and the stability lines at
different pressures. While the amplitude of the first harmonic is
fixed at
the pressure of the second harmonic is varied in 4 steps
from
to
. The large oscillations of the
stable bubble position as a function of the temporal phase is seen.
Their amplitudes increase
with increasing second harmonic driving pressure.
At
pressure the zero-force lines surround
small islands in the force landscape.
Also lines showing spatially unstable bubble behaviour are seen. The complexity
increases at
where multiple coexisting stability lines
are present with unstable connections. A
bubble can oscillate stably along the stability lines marked by filled symbols
and would sometimes jump by a discrete amount
if the temporal phase is changed.
FIG. 4 shows results for a bubble of
ambient radius. Different collapse
radii as a function of position and phase difference are shown together with the stability lines.
It is seen that the collapse radius changes along the stability lines. Bjerknes and
and buoyancy force keep the bubble away from regions with a very high energetic collapse.
In the multiple stability regime the
different bubble positions are associated with vastly different dynamics.
While at some points the bubble hardly oscillates others show
enormous compression rations needed for sonoluminescence.
Also shown are parametrically (surface) unstable bubbles [18]. Bubbles driven
at these phases/positions will show a dancing behaviour with less radial compression.
Next: Very High Frequency Modes
Up: Numerical Results
Previous: Dependence on Spatial Phase
Joachim Holzfuss
2004-10-04