Solar cycle 5
| Solar cycle 5 | |
|---|---|
| Sunspot Data | |
| Start date | May 1798 |
| End date | December 1810 |
| Duration (years) | 12.6 |
| Max count | 49.2 |
| Max count month | February 1805 |
| Min count | 0 |
| Cycle chronology | |
| Previous cycle | Solar cycle 4 (1784-1798) |
| Next cycle | Solar cycle 6 (1810-1823) |
The Dalton minimum in the 400-year history of sunspot numbers, showing the low peaks for solar cycles 5 and 6.
Solar cycle 5 was the fifth solar cycle since 1755, when extensive recording of solar sunspot activity began.[1][2] The solar cycle lasted 12.6 years, beginning in May 1798 and ending in December 1810 (thus falling within the Dalton Minimum). The maximum smoothed sunspot number (monthly number of sunspots averaged over a twelve-month period) observed during the solar cycle was 49.2, in February 1805 (the second-lowest of any cycle to date, as a result of being part of the Dalton Minimum), and the minimum was zero.[3]
See also
References
- ↑ Kane, R.P. (2002). "Some Implications Using the Group Sunspot Number Reconstruction". Solar Physics 205(2), 383-401.
- ↑ "The Sun: Did You Say the Sun Has Spots?". Space Today Online. Retrieved 12 August 2010.
- ↑ SIDC Monthly Smoothed Sunspot Number. ""
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