Chaotic ray dynamics in deep sea propagation models is considered using the
approaches developed in the theory of dynamical chaos. It has been demonst
rated that the mechanism of emergence of ray chaos due to overlapping of no
nlinear ray-medium resonances should play an important role in long range s
ound propagation. Analytical estimations, supported by numerical simulation
s, show that for realistic values of spatial periods and sound speed fluctu
ation amplitudes associated with internal-wave-induced perturbations, the r
esonance overlapping causes stochastic instability of ray paths. The influe
nce of the form of the smooth unperturbed sound speed profile on ray sensit
ivity to the perturbation is studied. Stability analysis has been conducted
by constructing the Poincare maps and examining depth differences of ray t
rajectories with close take-off angles. The properties of ray travel times,
including fractal properties of the time front fine structures, under cond
ition of ray chaos have been investigated. It has been shown that the coexi
stence of chaotic and regular rays, typical for dynamical chaos, leads to t
he appearance of gaps in ray travel time distributions, which are absent in
unperturbed waveguides. This phenomenon has a prototype in theory of dynam
ical chaos called the stochastic particle acceleration. It has been shown t
hat mesoscale inhomogeneities with greater spatial scales than that of inte
rnal waves, create irregular local waveguide channels in the vicinity of th
e axis (i.e., sound speed minimum) of the unperturbed waveguide. Near-axial
rays propagating at small grazing angles, "jump" irregularly between these
microchannels. This mechanism determines chaotic behavior of the near-axia
l rays.