Abstract
It is shown from the statistical analysis of the sunspot data and solar neutrino data that both the data exhibits 5, 10, 15, 20, 25, and 30 months period and these periods may be g-mode oscillation of the core associated with the solar activity.
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Raychaudhuri, P. Short-time variations of solar neutrinos and solar activity cycle. Sol Phys 106, 421–424 (1986). https://doi.org/10.1007/BF00158508
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DOI: https://doi.org/10.1007/BF00158508