Table 4
Observed and predicted SDO/AIA count rates for the jet spire and jet footpoint obtained using photospheric abundances.
Band | Observed | Predicted | Predicted | Observed | Predicted | Predicted | |
(Å) | (AIA-XRT DEM) | (EIS DEM) | (AIA-XRT DEM) | (EIS DEM) | |||
spire | spire | spire | footpoint | footpoint | footpoint | ||
|
|||||||
AIA 94 | 45 | 27 (–40%) | 10 (–78%) | 75 | 67 (–11%) | 22 (–71%) | |
AIA 131 | 303 | 244 (–20%) | 112 (–63%) | 455 | 350 (–23%) | 366 (–20%) | |
AIA 171 | 4747 | 5930 (25%) | 2134 (–55%) | 7651 | 7565 (–1%) | 5867 (–23%) | |
AIA 193 | 4494 | 5144 (15%) | 3181 (–29%) | 8063 | 7558 (–6%) | 6942 (–14%) | |
AIA 211 | 1946 | 1984 (2%) | 1461 (–25%) | 2957 | 2976 (1%) | 2891 (–2%) | |
AIA 335 | 117 | 101 (14%) | 59 (–50%) | 179 | 170 (–5%) | 116 (–35%) |
Notes. Columns 2 and 5 indicate the observed count rates (averaged DN/s per EIS pixel) for the region of the jet spire and the jet footpoint, respectively. Column 3, 4 and 6, 7 indicate predicted count rates obtained from the AIA-XRT DEM and EIS DEM for the region of the jet spire and the jet footpoint, respectively. Values in parenthesis in Cols. 3, 4 and 6, 7 show the percentage differences between observed and predicted intensities.
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