The Modern Maximum refers to the period of relatively high solar activity which began with Solar Cycle 15 in 1914. It reached a maximum in Cycle 19 during the late 1950s and may have ended with Cycle 23 in 2000 as Cycle 24 is recording, at best, very muted solar activity. This period is a natural example of solar variation, and one of many that are known from proxy records of past solar variability. The Modern Maximum reached a double peak once in the 1950s and again during the 1990s.
The value of the maximum, and even to some extent its existence, depends somewhat on the method of counting sunspot numbers.
- Ilya G. Usoskin, 4.4.1 The modern episode of active sun, A History of Solar Activity over Millennia, Living Reviews in Solar Physics (accessed 23 Sept. 2016).
- Rigozo, N. R.; Echer, E.; Vieira, L. E. A.; Nordemann, D. J. R. (2001). "Reconstruction of Wolf Sunspot Numbers on the Basis of Spectral Characteristics and Estimates of Associated Radio Flux and Solar Wind Parameters for the Last Millennium". Solar Physics. 203: 179–191. Bibcode:2001SoPh..203..179R. doi:10.1023/A:1012745612022.
- International Astronomical Union, Corrected sunspot history suggests climate change not due to natural solar trends, Phys.org, August 7, 2015 (accessed 23 Sept. 2016).
|This environment-related article is a stub. You can help Wikipedia by expanding it.|
|This article related to the Sun is a stub. You can help Wikipedia by expanding it.|