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  2. Sunspot - Wikipedia

    en.wikipedia.org/wiki/Sunspot

    Sunspots are temporary spots on the Sun's surface that are darker than the surrounding area. They are regions of reduced surface temperature caused by concentrations of magnetic flux that inhibit convection. Sunspots appear within active regions, usually in pairs of opposite magnetic polarity. [2] Their number varies according to the ...

  3. Sunspots (economics) - Wikipedia

    en.wikipedia.org/wiki/Sunspots_(economics)

    Sunspots (economics) In economics, the term sunspots (or sometimes "a sunspot") refers to an extrinsic random variable, that is, a random variable that does not affect economic fundamentals (such as endowments, preferences, or technology). Sunspots can also refer to the related concept of extrinsic uncertainty, that is, economic uncertainty ...

  4. Solar cycle - Wikipedia

    en.wikipedia.org/wiki/Solar_cycle

    The solar cycle, also known as the solar magnetic activity cycle, sunspot cycle, or Schwabe cycle, is a nearly periodic 11-year change in the Sun 's activity measured in terms of variations in the number of observed sunspots on the Sun's surface.

  5. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    The image shows light with a wavelength of 304 angstroms. Solar phenomena are natural phenomena which occur within the atmosphere of the Sun. They take many forms, including solar wind, radio wave flux, solar flares, coronal mass ejections, [1] coronal heating and sunspots. These phenomena are believed to be generated by a helical dynamo ...

  6. Sun in fiction - Wikipedia

    en.wikipedia.org/wiki/Sun_in_fiction

    Sunspots, and their 11-year cycle of frequency in occurrence, appear in a small number of works. The Sun poses a danger to spacecraft that approach it closely, a situation that occurs by necessity or design in several stories. It is sometimes depicted as being sentient, though this is rare compared to other stars getting the same treatment.

  7. Solar observation - Wikipedia

    en.wikipedia.org/wiki/Solar_observation

    From 2007 to 2009, sunspot levels were far below average. In 2008, the Sun was spot-free 73 percent of the time, extreme even for a solar minimum. Only 1913 was more pronounced, with no sunspots for 85 percent of that year. The Sun continued to languish through mid-December 2009, when the largest group of sunspots to emerge for several years ...

  8. Active region - Wikipedia

    en.wikipedia.org/wiki/Active_region

    In solar physics and observation, an active region is a temporary feature in the Sun's atmosphere characterized by a strong and complex magnetic field. They are often associated with sunspots and are commonly the source of violent eruptions such as coronal mass ejections and solar flares. [1] The number and location of active regions on the ...

  9. Solar maximum - Wikipedia

    en.wikipedia.org/wiki/Solar_maximum

    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 ...