“…When the instability threshold was slightly exceeded (10 mW < P 0 < 20 mW) the dependence of the BS signal on the pump power (figure 3(e)) was exponential, typical for convective decay instability [18,19]. However, at higher pump powers P 0 > 20 mW, even steeper dependence was observed in [20] indicating the absolute instability onset (see figure 3(e), curve 1). The absolute instability mechanism, according to [20], is related to the complicated spatial structure of the pump wave, namely, to the small fraction of the first radial mode present in the pump along with the dominant fundamental radial mode (P 1 0.1P 0 ) This small fraction interacting with the BS wave leads to the generation of the IA wave in the spatial point shifted by δz ∼ a from the main decay region.…”