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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. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    A solar flare is a sudden flash of brightness observed over the Sun's surface or the solar limb, which is interpreted as an energy release of up to 6 × 10 25 joules (about a sixth of the total Sun's energy output each second or 160 billion megatons of TNT equivalent, over 25,000 times more energy than released from the impact of Comet ...

  4. Sunlight - Wikipedia

    en.wikipedia.org/wiki/Sunlight

    The effect of Sun angle on climate results in the change in solar energy in summer and winter. For example, at latitudes of 65 degrees, this can vary by more than 25% as a result of Earth's orbital variation. Because changes in winter and summer tend to offset, the change in the annual average insolation at any given location is near zero, but ...

  5. Sunspot - Wikipedia

    en.wikipedia.org/wiki/Sunspot

    Sunspots themselves, in terms of the magnitude of their radiant-energy deficit, have a weak effect on solar flux. [39] The total effect of sunspots and other magnetic processes in the solar photosphere is an increase of roughly 0.1% in brightness of the Sun in comparison with its brightness at the solar-minimum level.

  6. Solar luminosity - Wikipedia

    en.wikipedia.org/wiki/Solar_luminosity

    Evolution of the solar luminosity, radius and effective temperature compared to the present-day Sun. After Ribas (2010) [1] The solar luminosity (L ☉) is a unit of radiant flux (power emitted in the form of photons) conventionally used by astronomers to measure the luminosity of stars, galaxies and other celestial objects in terms of the output of the Sun.

  7. Albedo - Wikipedia

    en.wikipedia.org/wiki/Albedo

    Another albedo-related effect on the climate is from black carbon particles. The size of this effect is difficult to quantify: the Intergovernmental Panel on Climate Change estimates that the global mean radiative forcing for black carbon aerosols from fossil fuels is +0.2 W m −2 , with a range +0.1 to +0.4 W m −2 . [ 63 ]

  8. Climate change is ending the Sun Belt boom - AOL

    www.aol.com/finance/climate-change-ending-sun...

    But Sun Belt migration is now skidding to a halt, according to a new working paper from the Federal Reserve Bank of San Francisco. As climate change makes warm places hotter and cold places more ...

  9. Effect of Sun angle on climate - Wikipedia

    en.wikipedia.org/wiki/Effect_of_Sun_angle_on_climate

    One of the first to publish on these effects was Milutin Milanković; the cyclic effects of axial tilt, eccentricity, and other orbital parameters upon global climate were named Milanković cycles. Although individual mechanisms (such as axial tilt and sun angle) are thought to be understood, the overall impact of orbital forcing on global ...