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 language | English |
|---|---|
| Pages (from-to) | L99-L101 |
| Journal | Astrophysical Journal |
| Volume | 673 |
| Issue number | 1 PART 2 |
| DOIs | |
| State | Published - 2008 |
Keywords
- Sun: activity
- Sun: magnetic fields
- Sun: photosphere