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  2. Solar wind - Wikipedia

    en.wikipedia.org/wiki/Solar_wind

    Ulysses's observations of solar wind speed as a function of helio latitude during solar minimum. Slow wind (≈ 400 km/s) is confined to the equatorial regions, while fast wind (≈ 750 km/s) is seen over the poles. [1] Red/blue colors show outward/inward polarities of the heliospheric magnetic field. An illustration of the structure of the Sun

  3. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    The finding that solar activity was approximately the same in cycles 14 and 24 applies to all solar outputs that have, in the past, been proposed as a potential cause of terrestrial climate change and includes total solar irradiance, cosmic ray fluxes, spectral UV irradiance, solar wind speed and/or density, heliospheric magnetic field and its ...

  4. August 1972 solar storms - Wikipedia

    en.wikipedia.org/wiki/August_1972_solar_storms

    Astronomers first reported unusual flares on 2 August, later corroborated by orbiting spacecraft. On 3 August, Pioneer 9 detected a shock wave and sudden increase in solar wind speed [33] from approximately 217–363 mi/s (349–584 km/s). [34] A shockwave passed Pioneer 10, which was 2.2 AU from the Sun at the time. [4]

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

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

    This relentless high-speed flow of charged particles from the sun fills interplanetary space. ... But precisely how the sun generates the solar wind has remained unclear. ... Climate change added ...

  6. Formation and evolution of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Formation_and_evolution_of...

    They will continue to orbit their star, their speed slowed due to their increased distance from the Sun and the Sun's reduced gravity. Two billion years later, when the Sun has cooled to the 6,000–8,000 K (5,730–7,730 °C; 10,340–13,940 °F) range, the carbon and oxygen in the Sun's core will freeze, with over 90% of its remaining mass ...

  7. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The heliosphere, the tenuous outermost atmosphere of the Sun, is filled with solar wind plasma and is defined to begin at the distance where the flow of the solar wind becomes superalfvénic—that is, where the flow becomes faster than the speed of Alfvén waves, [87] at approximately 20 solar radii (0.1 AU). Turbulence and dynamic forces in ...

  8. History-making NASA probe flies closer to the sun than ever ...

    www.aol.com/news/history-making-nasa-probe-flies...

    The Parker Solar Probe passed within just 3.8 million miles of the sun's surface — seven times ... closer to the sun than ever before — and breaks speed record. ... the solar wind’s ...

  9. List of solar cycles - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_cycles

    Solar cycles are nearly periodic 11-year changes in the Sun's activity that are based on the number of sunspots present on the Sun's surface. The first solar cycle conventionally is said to have started in 1755. The source data are the revised International Sunspot Numbers (ISN v2.0), as available at SILSO. [1]