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All p-mode parameters vary with time as a response to the changes induced bythe cyclic behavior of solar magnetic activity. After the unusual longsolar-activity minimum between cycles 23 and 24, where the p-mode parametershave shown a different behavior than the surface magnetic proxies, we analyzethe temporal variation of low-degree p-mode parameters measured by GOLF (invelocity) and VIRGO (in intensity) Sun-as-a-star instruments on board SoHO. Wethen compared our results with other activity proxies.

Towards solar activity maximum 24 as seen by GOLF and VIRGO/SPM instruments