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  2. List of solar cycles - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_cycles

    3-11 10-6 Solar cycle 20: 1964 – Oct 14.3 1968 – Nov 157 86 4-1 11-5 Solar cycle 21: 1976 – Mar 17.8 1979 – Dec 233 111 3-9 10-6 Solar cycle 22: 1986 – Sep 13.5 1989 – Nov 213 106 3-2 9-11 Solar cycle 23: 1996 – Aug 11.2 2001 – Nov 180 82 5-3 12-4 Solar cycle 24: 2008 – Dec 2.2 2014 – Apr 116 49 5-4 11-0 Solar cycle 25: 2019 ...

  3. Wilson effect (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Wilson_effect_(astronomy)

    Sunspots result from the blockage of convective heat transport by intense magnetic fields. Sunspots are cooler than the rest of the photosphere, with effective temperatures of about 4,000°C (about 7,000°F). Sunspot occurrence follows an approximately 11-year period known as the solar cycle, discovered by Heinrich Schwabe in the 19th century.

  4. Solar cycle - Wikipedia

    en.wikipedia.org/wiki/Solar_cycle

    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]

  5. The sun is at its 11-year maximum. That means another year of ...

    www.aol.com/sun-11-maximum-means-another...

    The sun emits the largest solar flare of this 11-year cycle, as imaged by NASA's Solar Dynamics Observatory on October 3. NASA/SDO NASA says the sun is in the highly active "maximum phase" of its ...

  6. Blast of energy from Sun triggers ongoing geomagnetic storm - AOL

    www.aol.com/blast-energy-sun-triggers-ongoing...

    NOAA and Nasa revealed the Sun reached solar maximum, a period of peak sunspot activity in its 11-year cycle. However, space weather experts said peak activity is expected to continue into 2025.

  7. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The largest sunspots can be tens of thousands of kilometers across. [111] An 11-year sunspot cycle is half of a 22-year Babcock–Leighton dynamo cycle, which corresponds to an oscillatory exchange of energy between toroidal and poloidal solar magnetic fields. At solar-cycle maximum, the external poloidal dipolar magnetic field is near its ...

  8. Babcock model - Wikipedia

    en.wikipedia.org/wiki/Babcock_Model

    At a solar-cycle minimum, the toroidal field is, correspondingly, at minimum strength, sunspots are few in number, and the poloidal field is at its maximum strength. With the rise of the next 11-year sunspot cycle, magnetic energy shifts back from the poloidal to the toroidal field, but with a polarity that is opposite to the previous cycle.

  9. Second major solar storm of year hits Earth as sunspot cycle ...

    www.aol.com/second-major-solar-storm-hits...

    The outburst marks the second of its kind this year after decades of relative calm — part of a cycle of increasing storms that… Second major solar storm of year hits Earth as sunspot cycle ...