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The parameters of the p-mode oscillations vary with solar activity. Suchtemporal variations provide insights for the study of the structural anddynamical changes occurring in the Sun's interior throughout the solar cycle.We present here a complete picture of the temporal variations of the globalp-mode parameters (excitation, damping, frequency, peak asymmetry, androtational splitting) over the entire solar cycle 23 and the beginning of cycle24 as observed by the space-based, Sun-as-a-star helioseismic GOLF and VIRGOinstruments onboard SoHO.

Global p-mode oscillations throughout the complete solar cycle 23 and the beginning of cycle 24