In this paper, we provide a complete geometrical treatment of classical rays emanating from an underwater point source and propagating in an unbounded medium where the speed of sound has a hyperbolic cosine dependence on the depth coordinate $(z)$ . General results are derived exclusively from Snell's law and are not limited to the case in which the ray emitting source is located at a point on the minimum propagation speed plane. Explicit relations are provided for the following: 1) the ray depth coordinate $(z)$ expressed as a function of the ray horizontal range $(\rho)$ and the ray source angle $(\theta_0)$ ; 2) all the relations among the ray source angle $(\theta_0)$ , the ray receiver angle $(\theta)$ , and the travel time $(\tau)$ to reach an arbitrary position of the receiver from an arbitrary position of the source; and 3) the classical wavefront coordinates $(\rho,z)$ along a ray expressed as a function of the ray source angle $(\theta_0)$ and travel time $(\tau)$ . From the wavefront coordinates $(\rho,z)$ , we construct and display ray/wavefront diagrams for a varying source depth $(z_0)$ relative to the minimum propagation speed plane. We also derive the time-averaged acoustic energy flux carried along classical ray tubes.
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