Fig. 11.


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(a) Plot of the estimated ρi using CCA on data segregated by Mount Wilson classes for i = 1, …, 9 within the sunspots α groups start out with the highest correlation. (b) Canonical patches a1 (top) and b1 (bottom) for the Mount Wilson classes within the sunspots. Again, the b1s are approximately equal to the negative of the a1s as in Figure 10 but the patches differ slightly from class to class.

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