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Fig. 6

image

Solar cycle peak amplitudes as a function of peak times (dots and solid lines) and rise amplitudes as a function of rise times (crosses and dashes lines) for each latitudinal band in the northern (left panels) and the southern (right panels) hemispheres for each solar cycle. The bars show the 99% confidence intervas. The colour coding for each latitudinal bands is the same with Fig. 4.

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