Solar cycle 20 was the twentieth solar cycle since 1755, when extensive recording of solar sunspot activity began.[2][3] The solar cycle lasted 11.4 years, beginning in October 1964 and ending in March 1976. The maximum smoothed sunspot number observed during the solar cycle was 156.6 (November 1968), and the starting minimum was 14.3.[4] During the minimum transit from solar cycle 20 to 21, there were a total of 272 days with no sunspots.[5][6][7]
Comparison with other cycles shows that geomagnetic activity during the declining phase of cycle 20 (1973–1975) was unusually high.[8] Heavy solar activity was a factor in causing the earlier-than-expected atmospheric reentry of Skylab in 1979.[9]
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.[10]
^Martin, James. "NASA celebrates the 40th anniversary of Skylab (pictures)". CNET. Retrieved 19 March 2022.
^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]"
^Spotless Days. "[2]"
^Dr. Tony Phillips (11 July 2008). "What's Wrong with the Sun? (Nothing)". NASA. Archived from the original on 14 July 2008.
^Solaemon's Spotless Days Page. "[3]"
^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.
^Benson, Charles Dunlap & Compton, William David (1983). Living and Working in Space: A History of Skylab. NASA Scientific and Technical Information Office. p. 362–363. OCLC 8114293. SP-4208.
^Miroshnichenko, Leonty (2001). Solar Cosmic Rays. Springer. p. 395. ISBN 0792369289.
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