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This is interesting from the point of view of the microphysics: do flares with no obvious opening of the field actually participate physically in maintaining the sector-boundary definition? 6 Long-Term Evolution of the Sector Structure The long-term behavior of the solar magnetic field, extending many Hale cycles into the past, has theoretical as well as practical interest (the latter since some prediction techniques involve solar activity with patterns whose “memory” extends to the preceding cycle or even earlier).

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G. F. Martyn, Electric currents in the ionosphere. I. The conductivity. R. Soc. Lond. Philos. Trans. Ser. A 246, 281–294 (1953). 0016 A. Balogh, G. Erd˝os, The heliospheric magnetic field. Space Sci. Rev. 176, 177–215 (2013). 1007/s11214-011-9835-3 B. Bell, A long-term North-South asymmetry in the location of solar sources of great geomagnetic storms. Smithson. Contrib. Astrophys. 5, 187 (1962) L. Biermann, Solar corpuscular radiation and the interplanetary gas. M. Borrero, K. Ichimoto, Magnetic structure of sunspots.

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