The longitudinal distribution of sunspots and the RS CVn starspot model

The longitudinal distribution of the sunspots has been investigated by using the observations made at the University Observatory of Istanbul in 1979. In order to take into account the activity as a whole, we obtained a new weighting system which depends on the area of spots and used it in our calculations. Differential rotation appeared to effect the considered distribution. It was determined that this longitudinal distribution of spots is not uniform but forms two maxima for two different longitudes. The obtained result verifies one of the main assumptions had been proposed in the starspot model in which accounts for the distortion wave appeared in the light curves of RS CVn-type binaries.