Revision history of "EVE Observations of Flare Footpoints"

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  • (cur | prev) 12:03, 22 November 2013 MichaelKennedy (Talk | contribs) (8,032 bytes) (Created page with "== Introduction == Impulsive emission during solar flares is typically observed at optical and UV wavelengths in the form of ribbons or footpoints in the chromosphere, as well a...")
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