Table 2
Observed and predicted XRT count rates for the active region area shown in Fig. 1.
Observed | Predicted | ||||
Photospheric 1 | Photospheric 2 | Coronal 1 | Coronal 2 | ||
|
|||||
Al_poly | 12 100 | 24 400 (+102%) | 21 600 (+79%) | 14 000 (+16%) | 16 200 (+34%) |
Al_thick | 22.2 | 30.6 (+38%) | 30.3 (+36%) | 17.5 (–21%) | 24.0 (+8%) |
Al_Ti | 4160 | 7770 (+87%) | 7080 (+70%) | 4560 (+10%) | 5360 (+29%) |
Be_thin | 2480 | 5050 (+104%) | 4660 (+88%) | 2940 (+19%) | 3500 (+41%) |
Be_med | 540 | 1020 (+89%) | 970 (+80%) | 572 (+6%) | 739 (+37%) |
Be_thick | 0.715 | 1.07 (+50%) | 1.17 (+64%) | 0.629 (–12%) | 0.923 (+29%) |
C_poly | 8410 | 16 100 (+91%) | 14 500 (+72%) | 9540 (+13%) | 11 000 (+31%) |
Ti_poly | 5667 | 10 500 (+85%) | 9490 (+67%) | 6090 (+7%) | 7290 (+29%) |
Notes. The predicted XRT count rates are determined from the corresponding EIS DEM curve. All values are in units of DN s-1 pix-1. Photospheric 1 and 2 correspond to the photospheric abundances of Grevesse et al. (1998) and Asplund et al. (2009) respectively. Coronal 1 corresponds to the coronal abundances of Feldman et al. (1992). Coronal 2 corresponds to the photospheric abundances of Asplund et al. (2009) with the oxygen and neon abundances reduced by a factor of three. The percentage difference between the observed and predicted count rates are included in parentheses.
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