| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.33 | 310.69 | 29.23 | 161.24 | 17.59 | 223.31 | -6.60 | 21.59 | 0.2991 | -746.6 | -362.7 | |
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back to the solar disc SDO HMI 2011-11-26 03:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.23 | 0.00 | 1.16 | 18.75 | 227.52 | -2.39 | 7.61 | 0.2997 | -850.0 | -636.2 | |
| 0.00 | 2.40 | 0.00 | 1.25 | 19.02 | 225.64 | -4.28 | 13.20 | 0.3099 | 895.0 | 704.4 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 18.84 | 225.58 | -4.33 | 13.52 | 0.3072 | 1027.0 | 801.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.12 | 225.48 | -4.43 | 13.60 | 0.3121 | 761.0 | 557.2 | |
| 0.51 | 1.80 | 0.27 | 0.94 | 19.18 | 224.75 | -5.16 | 15.66 | 0.3161 | 749.8 | 499.4 | |
| 17.04 | 249.56 | 8.81 | 129.37 | 17.23 | 223.88 | -6.03 | 20.37 | 0.2898 | -1315.6 | -425.8 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 19.73 | 223.66 | -6.25 | 18.17 | 0.3301 | -1033.0 | -695.5 | |
| 29.45 | -6.00 | 15.29 | -6.00 | 17.66 | 223.30 | -6.61 | 21.56 | 0.2999 | -1279.2 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 16.89 | 222.27 | -7.64 | 25.67 | 0.2951 | -750.0 | -471.9 | |
| 9.33 | 39.13 | 4.86 | 20.40 | 17.87 | 222.07 | -7.84 | 24.78 | 0.3112 | -1053.9 | -345.3 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.62 | 221.86 | -8.05 | 25.71 | 0.3090 | -881.0 | -734.4 | |
| 0.00 | 1.88 | 0.00 | 0.98 | 17.56 | 221.64 | -8.27 | 26.40 | 0.3097 | -709.0 | -523.0 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 15.14 | 221.56 | -8.35 | 30.78 | 0.2752 | 943.0 | 818.5 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 15.48 | 221.33 | -8.58 | 30.82 | 0.2819 | 975.0 | 799.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 15.72 | 221.23 | -8.68 | 30.66 | 0.2863 | 901.0 | 735.9 | |
| 0.00 | 2.05 | 0.00 | 1.08 | 18.60 | 220.08 | -9.83 | 28.86 | 0.3369 | 964.0 | 766.2 | |
| 0.00 | 1.46 | 0.00 | 0.77 | 18.82 | 219.78 | -10.13 | 29.25 | 0.3423 | 800.0 | 665.6 | |
| 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. | |