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  2. Solar wind - Wikipedia

    en.wikipedia.org/wiki/Solar_wind

    The solar wind is observed to exist in two fundamental states, termed the slow solar wind and the fast solar wind, though their differences extend well beyond their speeds. In near-Earth space, the slow solar wind is observed to have a velocity of 300–500 km/s , a temperature of ~ 100 kilokelvin and a composition that is a close match to the ...

  3. Van Allen radiation belt - Wikipedia

    en.wikipedia.org/wiki/Van_Allen_radiation_belt

    The Van Allen radiation belt is a zone of energetic charged particles, most of which originate from the solar wind, that are captured by and held around a planet by that planet's magnetosphere. Earth has two such belts, and sometimes others may be temporarily created.

  4. Solar wind turbulence - Wikipedia

    en.wikipedia.org/wiki/Solar_wind_turbulence

    Solar wind turbulence displays both magnetohydrodynamic (MHD) and kinetic plasma behaviors. It exhibits Kolmogorov-like power spectra at fluid scales, and shows strong Alfvénic correlations between velocity and magnetic field fluctuations, especially in fast solar wind. It evolves with distance from the Sun as the wind expands.

  5. Sun-observing spacecraft sheds light on the solar wind's origin

    www.aol.com/news/sun-observing-spacecraft-sheds...

    The solar wind is a ubiquitous feature of our solar system. ... Earth's magnetic field and atmosphere act as shields and protects life by blocking harmful particles and radiation from the sun. But ...

  6. Solar particle event - Wikipedia

    en.wikipedia.org/wiki/Solar_particle_event

    Post-eruptive loops in the wake of a solar flare, image taken by the TRACE satellite (photo by NASA). In solar physics, a solar particle event (SPE), also known as a solar energetic particle event or solar radiation storm, [a] [1] is a solar phenomenon which occurs when particles emitted by the Sun, mostly protons, become accelerated either in the Sun's atmosphere during a solar flare or in ...

  7. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    The solar wind is divided into the slow solar wind and the fast solar wind. The slow solar wind has a velocity of about 400 kilometres per second (250 mi/s), a temperature of 2 × 10 5 K and a composition that is a close match to the corona. The fast solar wind has a typical velocity of 750 km/s, a temperature of 8 × 10 5 K and nearly matches ...

  8. Solar power has exploded in popularity as wind lags, report shows

    www.aol.com/news/solar-power-exploded-popularity...

    A new trend for 2024 was diversification of these purchases to include not just wind and solar but also nuclear. Electric vehicle sales reached 1.5 million in 2024 , growing by 6.5%.

  9. Weather Words: Solar Wind

    www.aol.com/weather-words-solar-wind-140452877.html

    These wind events are called solar winds and are a key component of space weather. Solar winds are electrically charged particles emitted from the sun that are mostly made up of protons and electrons.