Table 2.
Observed and predicted (using EIS DEM) Hinode XRT count rates.
| Filter | Observed | Phot. | Phot. | Phot. | Coronal |
|---|---|---|---|---|---|
| increased | decreased | ||||
| Ti-poly | 14360 | 9328 | 9749 | 9303 | 7006 |
| Be-thin | 7380 | 4589 | 4897 | 4589 | 3420 |
Notes. The Phot. values are obtained with photospheric abundances. The last column shows the values with coronal abundances, where Fe is increased by a factor of about four (Feldman et al. 1992). The “increased” (and “decreased”) values are those obtained when the DEM at log T = 7.1 is increased (or decreased) by a factor of ten.
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