Wolf number

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Wolf number since 1750.

The Wolf number (also known as the International sunspot number, relative sunspot number, or Zürich number) is a quantity that measures the number of sunspots and groups of sunspots present on the surface of the sun.

The idea of computing sunspot numbers was originated by Rudolf Wolf in 1848[1] in Zurich, Switzerland and, thus, the procedure he initiated bears his name (or place). The combination of sunspots and their grouping is used because it compensates for variations in observing small sunspots.

This number has been collected and tabulated by researchers for over 150 years. They have found that sunspot activity is cyclical and reaches its maximum around every 9.5 to 11 years (note: Using data from SIDC for the last 300 years and running a FFT function on the data gives an average maximum at 10.4883 years/cycle).[2] This cycle was first noted by Heinrich Schwabe in 1843.

The relative sunspot number R is computed using the formula (collected as a daily index of sunspot activity):

R = k(10g + s) \,


  • s is the number of individual spots,
  • g is the number of sunspot groups, and
  • k is a factor that varies with location and instrumentation (also known as the observatory factor or the personal reduction coefficient K).[3]

Since 1 July 2015 a revised and updated list of the (Wolf) sunspot numbers has been made available,[4] although the revised series is not yet verified and is still subject to intensive debates.[citation needed]

See also[edit]


  1. ^ "The Sun - History". 2001-11-25. Retrieved 2012-01-08. 
  2. ^ SIDC, RWC Belgium, World Data Center for the Sunspot Index, Royal Observatory of Belgium, 'year(s)-of-data'.
  3. ^ personal reduction coefficient K
  4. ^ Switching to the new Sunspot Number (1 July 2015)

External links[edit]