Grand Solar Minimums and Maximums
Grand solar minimums occur when several solar cycles exhibit lesser than average activity for decades or centuries. Solar cycles still occur during these grand solar minimum periods but the intensity of those cycles are less intense. Grand solar minimums have shown some correlation with global and regional climate changes.
| Event | Start | End |
|---|---|---|
| Homeric minimum | 950BC | 800BC |
| Oort minimum (see Medieval Warm Period) | 1040 | 1080 |
| Medieval maximum (see Medieval Warm Period) | 1100 | 1250 |
| Wolf minimum | 1280 | 1350 |
| Spörer Minimum | 1450 | 1550 |
| Maunder Minimum | 1645 | 1715 |
| Dalton Minimum | 1790 | 1820 |
| Modern Maximum | 1900 | present |
A list of historical Grand minima of solar activity includes also Grand minima ca. 690 AD, 360 BC, 770 BC, 1390 BC, 2860 BC, 3340 BC, 3500 BC, 3630 BC, 3940 BC, 4230 BC, 4330 BC, 5260 BC, 5460 BC, 5620 BC, 5710 BC, 5990 BC, 6220 BC, 6400 BC, 7040 BC, 7310 BC, 7520 BC, 8220 BC, 9170 BC.
Read more about this topic: Solar Minimum
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