The waldmeier effect: An artifact of the definition of wolf sunspot number?

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Abstract

We show that the well-known "Waldmeier effect," or anticorrelation between the peak in sunspot number of a cycle and the time from minimum to reach that peak, is not present in sunspot area data averaged in the same way. With a 13-rotation Gaussian running average applied to both sunspot number and sunspot area, we find the correlation between cycle rise time and cycle peak is r = -0.71 for sunspot number and r = 10-4 for sunspot number. Thus the Waldmeier effect may be specific to only Wolf sunspot number.

Original languageEnglish
Pages (from-to)L99-L101
JournalAstrophysical Journal
Volume673
Issue number1 PART 2
DOIs
StatePublished - 2008

Keywords

  • Sun: activity
  • Sun: magnetic fields
  • Sun: photosphere

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