File:99 Overlapping-Cycles.png

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Figure 3. Four panels showing the decomposition of sunspot groups by cycle membership. This is unambiguously determined from their magnetic polarities. The bottom three panels show recent minimum periods; our current minimum (the very bottom) shows that the late arrival of new-cycle spots has allowed the number of old-cycle spots, and hence the total spot coverage, to be remarkably low.

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current19:13, 27 April 2010Thumbnail for version as of 19:13, 27 April 2010580×1,021 (42 KB)Hhudson (Talk | contribs) (Figure 3: Recent solar minima decomposed using the 'region days' analysis into their old-cycle and new-cycle components. Note that the earlier minima had much more overlap between cycles, and hence more activity during their shorter intervals.)
15:02, 12 April 2009Thumbnail for version as of 15:02, 12 April 2009577×1,013 (38 KB)Hhudson (Talk | contribs) (Figure 3. Four panels showing the decomposition of sunspot groups by cycle membership. This is unambiguously determined from their magnetic polarities. The bottom three panels show recent minimum periods; our current minimum (the very bottom) shows that )

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