The formation and the evolution of axisymmetric vortex rings in a unif
ormly rotating fluid, with the rotation axis orthogonal to the ring vo
rticity, have been investigated by numerical and laboratory experiment
s. The flow dynamics turned out to be strongly affected by the presenc
e of the rotation. In particular, as the background rotation increases
, the translation velocity of the ring decreases, a structure with opp
osite circulation forms ahead of the ring and an intense axial vortex
is generated on the axis of symmetry in the tail of the ring. The occu
rrence of these structures has been explained by the presence of a sel
f-induced swirl flow and by inspection of the extra terms in the Navie
r-Stokes equations due to rotation. Although in the present case the s
wirl was generated by the vortex ring itself, these results are in agr
eement with those of Virk et al. (1994) for polarized vortex rings, in
which the swirl flow was initially assigned as a 'degree of polarizat
ion'. If the rotation rate is further increased beyond a certain value
, the flow starts to be dominated by Coriolis forces. In this flow reg
ime, the impulse imparted to the fluid no longer generates a vortex ri
ng, but rather it excites inertial waves allowing the flow to radiate
energy. Evidence of this phenomenon is shown. Finally, some three-dime
nsional numerical results are discussed in order to justify some asymm
etries observed in flow visualizations.