Abstract
Using Greenwich sunspot data for 120 years it was recently observed that activity regions on the Sun's surface tend to lie along smoothly changing longitude strips 180° apart from each other. However, numerical experiments with random input data show that most, if not all, of the observed longitude discrimination can be an artifact of the analysis method.
| Original language | English |
|---|---|
| Pages (from-to) | 1093-1096 |
| Number of pages | 3 |
| Journal | Astronomy and Astrophysics |
| Volume | 429 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - Jan 2005 |
Keywords
- Methods: statistical
- Sun: activity
- Sun: magnetic fields
- Sun: sunspots
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