Revision history of "File:15 fe eqwidth.gif"

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  • (cur | prev) 01:24, 23 January 2010 Schriste (Talk | contribs) (278 bytes) (How the equivalent width of the Fe feature compares with theory for many points during a particular solar flare. Basically the flare evolution moves the points up in temperature rapidly, then more slowly downwards. At this level, the discrepancy is probab)
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