relative sunspot number A number devised by Rudolf Wolf of Zurich in 1849 to describe sunspot activity. Sometimes called the Wolf number, it is defined as: where R is the sunspot number, k is a constant depending on the instrument used, g is the number of disturbed regions, and f is the total number of sunspots. Related category SOLAR TOPICS Also on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History Transport Concepts & Designs (partner site) |