Solar cycle 20
Solar cycle 20 | |
---|---|
Solar magnetogram from solar cycle 20 (1974). | |
Sunspot Data | |
Start date | October 1964 |
End date | June 1976 |
Duration (years) | 11.7 |
Max count | 110.6 |
Max count month | November 1968 |
Min count | 12.2 |
Spotless days | 272 |
Cycle chronology | |
Previous cycle | Solar cycle 19 (1954-1964) |
Next cycle | Solar cycle 21 (1976-1986) |
Solar cycle 20 was the twentieth solar cycle since 1755, when extensive recording of solar sunspot activity began.[1][2] The solar cycle lasted 11.7 years, beginning in October 1964 and ending in June 1976. The maximum smoothed sunspot number (monthly number of sunspots averaged over a twelve-month period) observed during the solar cycle was 110.6 (November 1968), and the minimum was 12.2.[3] There were a total of 272 days with no sunspots during this cycle.[4][5][6]
Comparison with other cycles shows that geomagnetic activity during the declining phase of cycle 20 (1973–1975) was unusually high.[7]
Data from solar cycle 20 was used to build the K-1974 solar proton fluence model, used for planning space missions during solar cycle 21.[8]
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. ""
- ↑ Spotless Days. ""
- ↑ What's Wrong with the Sun? (Nothing) more information: Spotless Days. ""
- ↑ Solaemon's Spotless Days Page. ""
- ↑ Gosling, J. T.; Asbridge, J. R.; Bame, S. J. (1 August 1977). "An unusual aspect of solar wind speed variations during solar cycle 20". Journal of Geophysical Research 82 (22): 3311–3314. Bibcode:1977JGR....82.3311G. doi:10.1029/JA082i022p03311.
- ↑ Miroshnichenko, Leonty (2001). Solar Cosmic Rays. Springer. p. 395. ISBN 0792369289.
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