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'''Solar wind''' consists of particles, usually [[electron]]s and [[proton]]s, continually streaming away from the corona of the [[Sun]]. The solar wind has a magnetic field effect on [[cosmic rays]] and thus on [[cloud coverage]].<ref>[http://www.sepp.org/publications/NIPCC_final.pdf]
'''Solar wind''' consists of particles, usually [[electron]]s and [[proton]]s, continually streaming away from the corona of the [[Sun]]. The solar wind has a magnetic field effect on [[cosmic rays]] and thus on [[cloud coverage]].<ref>[http://www.sepp.org/publications/NIPCC_final.pdf]</ref>
The solar wind creates the Heliosphere, a bubble in the interstellar medium surrounding the [[solar system]]. Solar wind also creates the the [[aurora]] or "Northern Lights", and causes the tails of [[comet|comets]] to always point away from the sun.
The solar wind creates the Heliosphere, a bubble in the interstellar medium surrounding the [[solar system]]. Solar wind also creates the the [[aurora]] or "Northern Lights", and causes the tails of [[comet|comets]] to always point away from the sun.