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Solar wind

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NASA ScienceCasts: Effects of the Solar Wind

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What is Solar Wind?

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Solar Winds | How the Universe Works

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Solar Wind: A Silent Threat | Strip the Cosmos

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Jumper - Solar Wind

The solar wind is a stream of charged particles released from the upper atmosphere of the Sun, called the corona. This plasma consists of mostly electrons, protons and alpha particles with kinetic energy between 0.5 and 10 keV. Embedded within the solar-wind plasma is the interplanetary magnetic field. The solar wind varies in density, temperature and speed over time and over solar latitude and longitude. Its particles can escape the Sun's gravity because of their high energy resulting from the high temperature of the corona, which in turn is a result of the coronal magnetic field.
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