LATITUDE TIME DISTRIBUTION OF 3 TYPES OF MAGNETIC-FIELD ACTIVITY IN THE GLOBAL SOLAR-CYCLE

Large-scale solar activity is considered as a manifestation of 3 types of magnetic field activity which is demonstrated in the 22-year cycle (a) of small-scale flux emergence (polar faculae at latitudes > 40-degrees), (b) of somewhat larger scale flux emergence (sunspots at latitudes < 40-degrees), and (c) of the global magnetic neutral lines at all latitudes, The migration (poleward or equatorward) of the place of birth and/or of the phenomena themselves of these three types of manifestation of magnetic field is discussed. The poleward migration of the global field is explained in a phenomenological way.