期刊
出版社
IOP PUBLISHING LTD
DOI: 10.1088/1742-6596/440/1/012020
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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 compare our results with other activity proxies.
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