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  2. List of solar cycles - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_cycles

    Year 4 of SC25 (Dec 2022 to Nov 2023) averaged 41% more spots per day than year 4 of SC24. Year 5 of SC25 (Dec 2023 to Nov 2024) averaged 71% more spots per day than year 5 of SC24. Year 6 of SC25 (1 Dec 2024 to 3 Jan 2025) is currently averaging 27% more spots per day than at the same point in year 6 of SC24.

  3. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    [28] [42] Lockwood and Fröhlich, 2007, found "considerable evidence for solar influence on the Earth's pre-industrial climate and the Sun may well have been a factor in post-industrial climate change in the first half of the last century", but that "over the past 20 years, all the trends in the Sun that could have had an influence on the Earth ...

  4. Solar cycle - Wikipedia

    en.wikipedia.org/wiki/Solar_cycle

    Since observations began cycles as short as 9 years and as long as 14 years have been observed, and if the cycle of 1784–1799 is double then one of the two component cycles had to be less than 8 years in length. Significant amplitude variations also occur. Several lists of proposed historical "grand minima" of solar activity exist. [11] [20]

  5. Template:Distance from Sun using EasyTimeline - Wikipedia

    en.wikipedia.org/wiki/Template:Distance_from_Sun...

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us

  6. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    Ibn Yunus observed more than 10,000 entries for the Sun's position for many years using a large astrolabe. [184] The first reasonably accurate distance to the Sun was determined in 1684 by Giovanni Domenico Cassini. Knowing that directly measurements of the solar parallax were difficult, he chose to measure the Martian parallax.

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  8. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    The Earth's orbit varies between nearly circular and mildly elliptical (its eccentricity varies). When the orbit is more elongated, there is more variation in the distance between the Earth and the Sun, and in the amount of solar radiation, at different times in the year.

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