Similar as for Fig. 21, but for star CoRoT 102719279 (star No 9) in the LRA1. Only the stronger outburst at the middle of the light curve is analyzed. Three phases are found: (a) fading phase ↔, (b) relaxation phase ↔, and (c) relative quiescent phase ↔. As in the IR1, four groups of frequencies are present at 0.30, 1.12, 2.32, and 4.66 c d⁻¹ and their behavior from one phase to another is rather similar in the two runs, but their amplitude level is different.