SDO HMI 2011-08-08 15:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.99 | 22.10 | 1.03 | 11.65 | 20.12 | 221.59 | -13.48 | 40.23 | 0.3316 | -268.6 | -250.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.80 | 0.00 | 1.44 | 19.52 | 226.20 | -8.88 | 32.22 | 0.2740 | -566.0 | -660.9 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 19.61 | 225.93 | -9.14 | 32.79 | 0.2776 | -1025.0 | -765.6 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 19.02 | 225.80 | -9.27 | 34.42 | 0.2706 | -727.0 | -609.9 | |
| 1.99 | 2.53 | 1.03 | 1.31 | 20.70 | 225.63 | -9.44 | 31.44 | 0.2954 | -992.1 | -869.2 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 19.20 | 225.59 | -9.48 | 34.59 | 0.2751 | -829.0 | -678.1 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 20.32 | 225.30 | -9.77 | 33.07 | 0.2931 | -851.0 | -668.1 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 17.91 | 224.56 | -10.51 | 40.43 | 0.2688 | -747.0 | -506.5 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 19.12 | 224.39 | -10.68 | 37.97 | 0.2859 | -724.0 | -545.1 | |
| 0.00 | 2.53 | 0.00 | 1.33 | 20.81 | 221.58 | -13.49 | 40.64 | 0.3363 | -826.0 | -666.4 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 21.08 | 214.84 | -20.23 | 50.91 | 0.4174 | 768.0 | 557.9 | |
| 0.00 | 2.17 | 0.00 | 1.19 | 21.53 | 214.29 | -20.78 | 50.71 | 0.4282 | 713.0 | 602.3 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 22.28 | 214.07 | -21.00 | 49.55 | 0.4377 | 689.0 | 550.9 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 20.70 | 213.19 | -21.88 | 53.62 | 0.4348 | 673.0 | 542.4 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 18.34 | 212.04 | -23.03 | 59.64 | 0.4322 | 706.0 | 534.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |