Difference between revisions of "Coronal Mass Ejections"

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Revision as of 18:51, 11 October 2007

A Solar and Heliospheric Observatory (LASCO) observation of a CME.

Coronal Mass Ejections (CMEs) are a direct result of magnetic instabilities (i.e. solar flares) on the surface of the Sun erupting and expelling millions of tons of solar plasma into interplanetary space. CMEs are strongly influenced by the interplanetary magnetic field (IMF).


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