File:XRS fip models.jpg
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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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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 14:35, 1 November 2024 | | 801 × 473 (68 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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