In a collisionless magnetized argon plasma, a density cavity is produc
ed by the ponderomotive force that the transient radiation field of a
converging resonance cone exerts on the plasma. After the radiation fi
eld has decayed, the cavity develops into isotropic rarefactive densit
y waves that propagate at the ion sound velocity in the plasma. Since
the main density hole is well separated from the exciting structure, t
he propagation is not disturbed by the exciter antenna. The shape of t
he solitary density waves is determined by the opening angle of the co
ne and can, in a linear approximation, be described by a simple 3d wav
e equation. The propagation is apparently independent of the magnetic
field. Nonlinear features of wave propagation were studied by superimp
osing counterpropagating waves. A model for the spatio-temporal evolut
ion is presented.