Institution(s): 1. University of Turku
The current photometric datasets, that span decades, allow for studying long-term magentic cycles on active stars. Complementary Ca H&K observations give information also on the cycles of normal solar-like stars, which have significantly smaller, and less easily detectable, spots. In recent years, high precision space-based observations, for example from the Kepler satellite, have allowed also to study the sunspot-like spot sizes in other stars. In this talk I will review what is known about the properties of the cyclic stellar activity in other stars than our Sun, and also discuss the future prospects in this field.