Solar wind facts for kids

Ulysses' observations of solar wind speed as a function of helio latitude during solar minimum. Slow wind (≈7005400000000000000♠400 km/s) is confined to the equatorial regions, while fast wind (≈7005750000000000000♠750 km/s) is seen over the poles. Red/blue colors show inward/outward polarities of the heliospheric magnetic field.

The Solar Wind is wind from the sun. It is a stream of charged protons, electrons and plasma shot out of the Sun. The wind is shot out at hypersonic speed, so fast that it can travel the whole length of the Solar System, nearly 1 light year and create the heliosphere. The particles are dangerous to astronauts and spacecraft. The Earth's magnetic field absorbs or soaks up a lot of the solar wind causing the aurora, the Northern lights and Southern lights.

A disturbance in the solar wind is called a solar storm. Sometimes it causes a geomagnetic storm. Such a storm in 1989 brought down the Quebec electric power grid putting the entire province in darkness. The largest recorded geomagnetic storm was in September 1 – 2, 1859. If we were to have another as strong as that one it is estimated it would cause up to 2 trillion dollars damage.

Solar wind also causes the tail of a comet. When the comet is close enough to the sun that the heat evaporates some of the comet's ice, the motion of the solar wind causes the resulting water vapor and space dust to stream away from the comet. Because it is blown by the solar wind, the comet's tail does not trail behind it, but always points directly away from the sun.

Images for kids

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  Laboratory simulation of the magnetosphere's influence on the solar wind; these auroral-like Birkeland currents were created in a terrella, a magnetised anode globe in an evacuated chamber.

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  This is thought to show the solar wind from the star L.L. Orionis generating a bow shock (the bright Arc)

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  CME erupts from Earth's Sun

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  Parker Solar Probe observed switchbacks — traveling disturbances in the solar wind that caused the magnetic field to bend back on itself.

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  The heliospheric current sheet results from the influence of the Sun's rotating magnetic field on the plasma in the solar wind

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  Noon meridian section of magnetosphere

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  Apollo's SWC experiment

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  Apollo's Solar Wind Composition Experiment on the Lunar surface

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  An infographic featuring the outer regions of the heliosphere based on results from the Voyager spacecraft