Revisiting the hypothesis of purely stochastic excitation of global p modes in the Sun

Open Access

Fig. 7.

Distributions of normalised combined energies. For each cycle period, we show the histogram, the best $Γ_{k = 36, th}$ $\varGamma_{k = 36,\mathrm{th}}$ distribution in continuous line and its mean in dashed line. Red data correspond to low magnetic activity, the brown ones to high activity, the yellow ones to the maximum of cycle 23, and the green ones to the maximum of cycle 24.

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