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arxiv: 1301.6930 · v1 · pith:L6XIUUIAnew · submitted 2013-01-29 · 🌌 astro-ph.SR

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

R. A. Garcia , D. Salabert , S. Mathur , C. Regulo , J. Ballot , G.R. Davies , A. Jimenez , R. Simoniello This is my paper
classification 🌌 astro-ph.SR
keywords activityp-modeparametersbehaviorgolfinstrumentsmagneticproxies
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All p-mode parameters vary with time as a response to the changes induced by the cyclic behavior of solar magnetic activity. After the unusual long solar-activity minimum between cycles 23 and 24, where the p-mode parameters have shown a different behavior than the surface magnetic proxies, we analyze the temporal variation of low-degree p-mode parameters measured by GOLF (in velocity) and VIRGO (in intensity) Sun-as-a-star instruments on board SoHO. We then compared our results with other activity proxies.

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