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Fig. 1.

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Influence of the magnetic activity cycle on frequency separation ratios, r01 and r02, observed by BiSON. The grey data represent the averaged shift due to magnetic activity. The full frequency range was considered (n = 14 − 24). The red line was obtained by smoothing the grey data with a Savitzky-Golay filter. The 10.7 cm radio emission flux, a proxy of the solar cycle, is denoted in black. The correlation with the activity proxy is measured with the Spearman rank coefficient, ℛ.

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