Revision history of "File:XRS fip models.jpg"

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  • (cur | prev) 19:37, 22 October 2008 Schriste (Talk | contribs) (169 bytes) (FIP bias vs. FIP for two different models of coronal abundances used by CHIANTI and for the XRS-measured values for Fe, Ca, Si, and S averaged over five ~M-class flares.)
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