File:Coronal Mass Ejection.gif

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Original file ‎(2,048 × 2,048 pixels, file size: 1.62 MB, MIME type: image/gif, looped, 2 frames, 4.0 s)

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English: Arcs rise above an active region on the surface of the Sun in this series of images taken by the STEREO (Behind) spacecraft. The arcs are plasma, superheated matter made up of moving charged particles (electrons and ions). Just as iron filings arc from one end of a magnet to another, the plasma is sliding in an arc along magnetic field lines. Most coronal mass ejections are more bulbous and wide: this one is quite narrow and contained. Nonetheless, NASA solar scientists agree that its speed and characteristics suggest that it was indeed a non-typical coronal mass ejection.
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Source NASA Earth Observatory
Author Images courtesy of the STEREO Science Center

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current11:38, 15 February 2010Thumbnail for version as of 11:38, 15 February 20102,048 × 2,048 (1.62 MB)Originalwana (talk | contribs){{Information |Description={{en|1=Fiery arcs rise above an active region on the surface of the Sun in this series of images taken by the STEREO (Behind) spacecraft. The arcs are plasma, superheated matter made up of mov

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