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4-2 11-3 Solar cycle 11: 1867 – Mar 9.9 1870 – Aug 234 89 3-5 11-9 Solar cycle 12: 1878 – Dec 3.7 1883 – Dec 124 57 5-0 11-3 Solar cycle 13: 1890 – Mar 8.3 1894 – Jan 147 65 3-10 11-10 Solar cycle 14: 1902 – Jan 4.5 1906 – Feb 107 54 4-1 11-6 Solar cycle 15: 1913 – Jul 2.5 1917 – Aug 176 73 4-1 10-1 Solar cycle 16: 1923 ...
The sun emits the largest solar flare of this 11-year cycle, as imaged by NASA's Solar Dynamics Observatory on October 3. ... a 2023 study found that flights were 21% more likely to be delayed by ...
Solar maximum is the regular period of greatest solar activity during the Sun's 11-year solar cycle. During solar maximum, large numbers of sunspots appear, and the solar irradiance output grows by about 0.07%. [2] On average, the solar cycle takes about 11 years to go from one solar maximum to the next, with duration observed varying from 9 to ...
Solar cycle 23 lasted 11.6 years, beginning in May 1996 and ending in January 2008. The maximum smoothed sunspot number (monthly number of sunspots averaged over a twelve-month period) observed during the solar cycle was 120.8 (March 2000), and the minimum was 1.7. [29] A total of 805 days had no sunspots during this cycle. [30] [31] [32]
In 2002, Lean et al. [41] stated that while "There is ... growing empirical evidence for the Sun's role in climate change on multiple time scales including the 11-year cycle", "changes in terrestrial proxies of solar activity (such as the 14C and 10Be cosmogenic isotopes and the aa geomagnetic index) can occur in the absence of long-term (i.e ...
This index (also known as the Zürich number) uses both the number of sunspots and the number of sunspot groups to compensate for measurement variations. A 2003 study found that sunspots had been more frequent since the 1940s than in the previous 1150 years. [30] Sunspots usually appear as pairs with opposite magnetic polarity. [31]
The solar cycle spans approximately 11 years, from one solar minimum to the following minimum. Since the solar magnetic field is continually wound up due to the faster rotation of mass at the Sun's equator (differential rotation), sunspot activity is more pronounced at solar maximum where the magnetic field is more twisted.
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