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Solar cycle 2
| Field | Value |
|---|---|
| image | Wilson effect original.jpg |
| caption | Drawing of a sunspot from 1774, illustrating the Wilson effect |
| cycle_num | 2 |
| start_date | June 1766 |
| end_date | June 1775 |
| duration | 9 |
| max_count | 193.0 |
| max_count_date | September 1769 |
| min_count | 18.6 |
| prev_name | Solar cycle 1 |
| prev_dates | 1755–1766 |
| next_name | Solar cycle 3 |
| next_dates | 1775–1784 |
Solar cycle 2 was the second solar cycle since 1755, when extensive recording of sunspot activity began. The solar cycle lasted 9 years, beginning in June 1766 and ending in June 1775. The maximum smoothed sunspot number observed during the solar cycle was 193.0 (September 1769), and the starting minimum was 18.6.
Sunspot observations by Alexander Wilson during this period established the Wilson effect.
References
References
- (2002). "Some Implications Using the Group Sunspot Number Reconstruction". Solar Physics.
- "The Sun: Did You Say the Sun Has Spots?". Space Today Online.
- "SIDC Monthly Smoothed Sunspot Number".
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