Abstract
We review how the so-called flux-transport solar dynamos work and show that such models calibrate well with solar cycle observations, and simulate well the relative peaks of the past 8 cycles. This success provides a basis for forecasting a strong solar cycle 24. We also show that a previous forecast of the timing of onset of cycle 24 is being verified by recent sunspot area statistics and coronal structures.
| Original language | English |
|---|---|
| Pages (from-to) | 17-24 |
| Number of pages | 8 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 2 |
| Issue number | 233 |
| DOIs | |
| State | Published - Mar 2006 |
Keywords
- Sun: activity
- Sun: interior
- Sun: magnetic fields
- Sun: photosphere
- Sun: sunspots