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Solar wind

 Home Physics Concepts in physics Physical phenomena Stellar phenomena Solar phenomena
 0 By others on same topic  0 Discussions  1970-01-01  See my version
Solar wind is a continuous flow of charged particles, primarily electrons and protons, released from the upper atmosphere of the Sun, known as the corona. This stream of plasma travels through space at varying speeds, typically ranging from 300 to 800 kilometers per second (about 670,000 to 1.8 million miles per hour).

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