Solar cycle 6 was the sixth solar cycle since 1755, when extensive recording of solar sunspot activity began.[1][2] The solar cycle lasted 12.8 years, beginning in August 1810 and ending in May 1823 (thus falling within the Dalton Minimum). The maximum smoothed sunspot number observed during the solar cycle was 81.2, in May 1816 (the lowest of any cycle to date, as a result of being part of the Dalton Minimum), and the starting minimum was 0.0.[3]
| Solar cycle 6 | |
|---|---|
 | |
| Sunspot data | |
| Start date | August 1810 |
| End date | May 1823 |
| Duration (years) | 12.8 |
| Max count | 81.2 |
| Max count month | May 1816 |
| Min count | 0.0 |
| Cycle chronology | |
| Previous cycle | Solar cycle 5 (1798–1810) |
| Next cycle | Solar cycle 7 (1823–1833) |
See also
editReferences
edit- ^ Kane, R.P. (2002), "Some Implications Using the Group Sunspot Number Reconstruction", Solar Physics, 205 (2): 383–401, Bibcode:2002SoPh..205..383K, doi:10.1023/A:1014296529097
- ^ "The Sun: Did You Say the Sun Has Spots?". Space Today Online. Retrieved 12 August 2010.
- ^ SIDC Monthly Smoothed Sunspot Number. "[1]"
 | This article related to the Sun is a stub. You can help Wikipedia by expanding it. |