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Figure 2 | SpringerPlus

Figure 2

From: Large-scale solar magnetic field mapping: I

Figure 2

Same as Figure 1 but extended to a long run of 4,000 tick timesteps. A quiet period after ~3000 ticks can be seen, reminiscent of a Maunder minimum. One can also see the typical chaotic nature of the solar cycles calculated with this model. One may also discern the Waldmeier anti-correlation of cycle amplitude with cycle duration in Plot A.

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