| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.40 | 348.12 | 29.42 | 195.36 | -18.20 | 352.14 | 22.48 | 230.68 | 0.4717 | 1033.0 | 423.2 | |
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back to the solar disc SDO HMI 2011-12-15 21:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.49 | 321.50 | 24.96 | 180.44 | -18.00 | 352.24 | 22.58 | 231.13 | 0.4710 | 1340.4 | 416.1 | |
| 4.42 | -1.00 | 2.50 | -1.00 | -19.08 | 352.32 | 22.67 | 229.38 | 0.4818 | 937.7 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -18.96 | 351.76 | 22.11 | 228.92 | 0.4742 | 798.0 | 603.6 | |
| 0.00 | 1.11 | 0.00 | 0.61 | -16.23 | 350.75 | 21.10 | 232.58 | 0.4371 | -682.0 | -556.7 | |
| 3.49 | 13.10 | 1.96 | 7.34 | -19.46 | 350.99 | 21.34 | 227.12 | 0.4701 | 869.0 | 770.6 | |
| 0.00 | 1.53 | 0.00 | 0.86 | -19.96 | 350.89 | 21.24 | 226.18 | 0.4739 | 754.0 | 634.6 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -19.22 | 350.79 | 21.14 | 227.28 | 0.4654 | 882.0 | 747.9 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -19.68 | 350.85 | 21.20 | 226.59 | 0.4707 | 812.0 | 633.1 | |
| 0.00 | 1.70 | 0.00 | 0.97 | -21.40 | 351.07 | 21.42 | 224.13 | 0.4903 | 650.0 | 565.3 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -16.81 | 350.42 | 20.77 | 231.06 | 0.4383 | -733.0 | -602.3 | |
| 0.00 | 1.02 | 0.00 | 0.58 | -21.41 | 350.90 | 21.25 | 223.91 | 0.4885 | 787.0 | 582.0 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -20.15 | 350.52 | 20.86 | 225.38 | 0.4716 | 714.0 | 591.1 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -19.93 | 350.38 | 20.73 | 225.57 | 0.4680 | 943.0 | 739.9 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -17.80 | 350.08 | 20.42 | 228.81 | 0.4434 | -673.0 | -513.0 | |
| 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. | |