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  2. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    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 ...

  3. Day length fluctuations - Wikipedia

    en.wikipedia.org/wiki/Day_length_fluctuations

    Then this value is related to the corresponding change of the length of day Δτ (in milliseconds) as [citation needed] u ≈ 2.7 Δ τ . {\displaystyle u\approx 2.7\Delta \tau .} The annual component of the change of the length of day of Δ τ ≈ 0.34 ms corresponds then to a superrotation of u ≈ 0.9 m/s, and the semiannual component of Δ ...

  4. List of solar cycles - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_cycles

    As at Feb 20, 2025, solar cycle 25 is averaging 37% more spots per day than solar cycle 24 at the same point in the cycle (Feb 20, 2014). Year 1 of SC25 (Dec 2019 to Nov 2020) averaged 101% more spots per day than year 1 of SC24. Year 2 of SC25 (Dec 2020 to Nov 2021) averaged 7% more spots per day than year 2 of SC24.

  5. Solar irradiance - Wikipedia

    en.wikipedia.org/wiki/Solar_irradiance

    Losses depend on time of day (length of light's path through the atmosphere depending on the solar elevation angle), cloud cover, moisture content and other contents. The irradiance above the atmosphere also varies with time of year (because the distance to the Sun varies), although this effect is generally less significant compared to the ...

  6. Solar time - Wikipedia

    en.wikipedia.org/wiki/Solar_time

    On a prograde planet like the Earth, the sidereal day is shorter than the solar day. At time 1, the Sun and a certain distant star are both overhead. At time 2, the planet has rotated 360° and the distant star is overhead again (1→2 = one sidereal day). But it is not until a little later, at time 3, that the Sun is overhead again (1→3 = one solar day). More simply, 1→2 is a complete ...

  7. Winter solstice: The shortest day and longest night of the year

    www.aol.com/news/winter-solstice-shortest-day...

    The date that the solstice occurs can move forward or back by a day because the solar year (the time it takes for the sun to reappear in the same spot as seen from Earth) doesn’t match up ...

  8. Solar cycle - Wikipedia

    en.wikipedia.org/wiki/Solar_cycle

    2,300 year Hallstatt solar variation cycles. Periodicity of solar activity with periods longer than the solar cycle of about 11 (22) years has been proposed, including: The Hallstatt cycle (named after a cool and wet period in Europe when glaciers advanced) is hypothesized to extend for approximately 2,400 years. [54] [55] [56] [57]

  9. Tropical year - Wikipedia

    en.wikipedia.org/wiki/Tropical_year

    The length of the tropical year was given as 365 solar days 5 hours 49 minutes 16 seconds (≈ 365.24255 days). This length was used in devising the Gregorian calendar of 1582. [7] In Uzbekistan, Ulugh Beg's Zij-i Sultani was published in 1437 and gave an estimate of 365 solar days 5 hours 49 minutes 15 seconds (365.242535 days). [8]