SDO HMI 2011-08-07 09:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.86 | 57.32 | 5.57 | 29.56 | 18.96 | 241.59 | -10.02 | 36.25 | 0.2786 | 105.0 | 529.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.44 | 8.95 | 1.76 | 4.58 | 18.62 | 244.39 | -7.22 | 28.86 | 0.2478 | -1091.1 | -740.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 17.53 | 244.27 | -7.33 | 31.65 | 0.2330 | -918.0 | -717.5 | |
| 3.62 | -1.00 | 1.85 | -1.00 | 18.43 | 244.14 | -7.47 | 30.08 | 0.2471 | -1020.8 | 999999 | |
| 0.00 | 2.53 | 0.00 | 1.30 | 18.98 | 243.24 | -8.37 | 31.75 | 0.2627 | -838.0 | -477.1 | |
| 1.54 | 5.33 | 0.79 | 2.75 | 19.59 | 242.35 | -9.25 | 33.02 | 0.2791 | -593.2 | -707.4 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 18.02 | 241.92 | -9.68 | 37.76 | 0.2623 | 687.0 | 474.0 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 18.26 | 241.45 | -10.15 | 38.45 | 0.2703 | 988.0 | 709.6 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 18.38 | 241.25 | -10.35 | 38.70 | 0.2740 | 1018.0 | 772.3 | |
| 2.26 | 21.34 | 1.17 | 11.02 | 18.87 | 240.76 | -10.84 | 38.80 | 0.2853 | 1130.4 | 892.2 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 19.46 | 240.46 | -11.14 | 38.21 | 0.2959 | 942.0 | 794.4 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 18.99 | 240.43 | -11.18 | 39.35 | 0.2903 | 816.0 | 705.3 | |
| 0.00 | 8.41 | 0.00 | 4.37 | 19.74 | 240.34 | -11.26 | 37.89 | 0.3006 | 1063.0 | 815.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 18.79 | 239.89 | -11.72 | 41.12 | 0.2937 | 727.0 | 569.3 | |
| 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. | |