This paper explores the propagation and interaction mechanisms demonstrated by compressible vortex rings. With spark shadowgraph and schlieren photography, we examine the vortical flow regimes produced by the impulse of a shock wave emerging from the open end of a shock tube. For shock-wave Mach numbers ranging from M s = 1.0 to 2.0, three distinct flow regimes were identified. From M s = 1.0 to 1.43, conventional-looking vortex rings are produced. These vortex rings are characterized by very thin cores and thus high circumferential instability wavenumbers. From M s = 1.43 to 1.60, the axial flow velocity in the recirculating region of the vortex ring becomes supersonic, producing a rearward-facing shock wave embedded in this region. From M s = 1.60 to 2.0, a secondary counter-rotating vortex ring forms ahead of the main vortex-ring. Finally, preliminary results on the interaction of two compressible vortex rings are presented.
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Brouillette et al. (1997) studied this question.
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