We define the solar cycle as a spatiotemporal rather than a purely temporal
entity. This allows us to introduce new methods to determine timing parame
ters of the activity cycles. We discuss the physical interpretation of our
spatiotemporal definition as a pair of activity waves travelling towards th
e equator and pole respectively, and present results of the corresponding s
tatistical analysis. Three important trends of solar activity which are cle
arly seen in summary statistics can be used for prediction. We present evid
ence of a long term cycle of 90 years manifesting as a modulation of both l
ength and symmetry of the Schwabe cycle and identify this with the Gleissbe
rg cycle.