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  2. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    Solar storms are caused by disturbances on the Sun, most often coronal clouds associated with solar flare CMEs emanating from active sunspot regions, or less often from coronal holes. The Sun can produce intense geomagnetic and proton storms capable of causing power outages , disruption or communications blackouts (including GPS systems) and ...

  3. Solar radio emission - Wikipedia

    en.wikipedia.org/wiki/Solar_radio_emission

    Solar radio emission refers to radio waves that are naturally produced by the Sun, primarily from the lower and upper layers of the atmosphere called the chromosphere and corona, respectively. The Sun produces radio emissions through four known mechanisms, each of which operates primarily by converting the energy of moving electrons into ...

  4. Solar energy - Wikipedia

    en.wikipedia.org/wiki/Solar_energy

    In 2011, a report by the International Energy Agency found that solar energy technologies such as photovoltaics, solar hot water, and concentrated solar power could provide a third of the world's energy by 2060 if politicians commit to limiting climate change and transitioning to renewable energy. The energy from the Sun could play a key role ...

  5. Solar core - Wikipedia

    en.wikipedia.org/wiki/Solar_core

    The energy produced by fusion in the core, except a small part carried out by neutrinos, must travel through many successive layers to the solar photosphere before it escapes into space as sunlight, or else as kinetic or thermal energy of massive particles. The energy conversion per unit time (power) of fusion in the core varies with distance ...

  6. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The core is the only region of the Sun that produces an appreciable amount of thermal energy through fusion; 99% of the Sun's power is generated in the innermost 24% of its radius, and almost no fusion occurs beyond 30% of the radius. The rest of the Sun is heated by this energy as it is transferred outward through many successive layers ...

  7. Solar irradiance - Wikipedia

    en.wikipedia.org/wiki/Solar_irradiance

    Global map of global horizontal radiation [5] Global Map of Direct Normal Radiation [5]. There are several measured types of solar irradiance. Total solar irradiance (TSI) is a measure of the solar power over all wavelengths per unit area incident on the Earth's upper atmosphere.

  8. Solar eclipse myths explained: What to know about eclipse ...

    www.aol.com/solar-eclipse-myths-explained-know...

    The bananas on your counter produce neutrinos, too, according to the U.S. Department of Energy. A solar eclipse has no impact on the number of neutrinos produced by the sun, how they travel across ...

  9. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    The solar constant is defined for the Sun's radiation at the distance to the Earth, also known as one astronomical unit (au). Consequently, at a distance of R astronomical units (R thus being dimensionless), applying the inverse-square law, we would find: = ⁡.