  Through meticulous daily observation of the Sun's large-scale magnetic field
the Wilcox Solar Observatory (WSO) has catalogued two magnetic (Hale) cycles of
solar activity. Those two (~22-year long) Hale cycles have yielded four
($\sim$11-year long) sunspot cycles (numbers 21 through 24). Recent research
has highlighted the persistence of the "Extended Solar Cycle" (ESC) and its
connection to the fundamental Hale Cycle - albeit through a host of proxies
resulting from image analysis of the solar photosphere, chromosphere and
corona. This short manuscript presents the correspondence of the ESC, the
surface toroidal magnetic field evolution, and the evolution of the Hale Cycle.
As Sunspot Cycle 25 begins, interest in observationally mapping the Hale and
Extended cycles could not be higher given potential predictive capability that
synoptic scale observations can provide.
