Similar as for Fig. 21, but for star CoRoT102686433 (star No 6) in the LRA1. Five phases are found in the light curve: (a) relative quiescent phase 1 ↔, (b) precursor phase ↔, (c) brightening phase ↔, (d) relaxation phase ↔, and (e) relative quiescent phase 2 ↔ (upper left panel). Changes in amplitude of the five groups of frequencies at 1.15, 1.30, 2.27, 2.42, 2.60, 3.40, and 4.57 c d⁻¹ are seen between the different phases (right panels); errors of the amplitude estimates are ~ ±10% ppm on average. The behavior of the amplitudes of the two frequency groups at 1.30 and 2.60 c d⁻¹ in relaxation phase (d) and the relative quiescent phases (a) and (e) differs from that of the other groups.