SDO HMI 2011-11-24 23:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.86 | 433.77 | 44.60 | 227.03 | 15.26 | 232.45 | -12.84 | 41.55 | 0.3209 | -577.9 | -291.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.20 | 0.00 | 0.61 | 13.78 | 236.68 | -8.61 | 34.75 | 0.2562 | -926.0 | -703.3 | |
| 0.00 | 1.20 | 0.00 | 0.61 | 13.36 | 236.32 | -8.96 | 36.84 | 0.2540 | 681.0 | 490.3 | |
| 7.45 | 19.09 | 3.82 | 9.80 | 13.60 | 235.57 | -9.71 | 38.45 | 0.2649 | -1139.9 | -702.3 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 13.32 | 234.88 | -10.41 | 41.06 | 0.2689 | -885.0 | -731.1 | |
| 0.00 | 1.97 | 0.00 | 1.03 | 16.76 | 234.58 | -10.71 | 34.36 | 0.3166 | -891.0 | -601.6 | |
| 0.00 | 2.23 | 0.00 | 1.17 | 17.31 | 234.26 | -11.02 | 34.12 | 0.3270 | -917.0 | -814.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 12.90 | 234.40 | -10.89 | 43.41 | 0.2691 | -939.0 | -813.3 | |
| 48.72 | 296.42 | 25.26 | 153.67 | 14.99 | 234.27 | -11.02 | 38.73 | 0.2965 | -1441.6 | -434.5 | |
| 1.63 | -8.00 | 0.85 | -8.00 | 15.16 | 233.70 | -11.59 | 39.73 | 0.3048 | -776.8 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.49 | 233.40 | -11.89 | 35.79 | 0.3375 | -784.0 | -671.4 | |
| 0.68 | 1.88 | 0.36 | 0.98 | 14.97 | 232.36 | -12.93 | 43.19 | 0.3172 | -995.0 | -838.9 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 14.76 | 232.09 | -13.20 | 44.25 | 0.3178 | -762.0 | -660.2 | |
| 0.00 | 2.05 | 0.00 | 1.08 | 16.50 | 231.78 | -13.50 | 41.16 | 0.3417 | -889.0 | -670.2 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.44 | 231.46 | -13.83 | 39.96 | 0.3566 | -710.0 | -615.7 | |
| 1.46 | 3.34 | 0.78 | 1.78 | 18.43 | 231.28 | -14.00 | 38.50 | 0.3704 | -827.3 | -690.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 14.82 | 231.55 | -13.74 | 45.24 | 0.3248 | -866.0 | -711.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 16.49 | 231.43 | -13.85 | 41.87 | 0.3454 | -890.0 | -704.5 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.41 | 231.24 | -14.05 | 40.46 | 0.3585 | -760.0 | -624.5 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 16.37 | 231.22 | -14.07 | 42.55 | 0.3463 | -901.0 | -649.1 | |
| 0.00 | 2.14 | 0.00 | 1.13 | 16.61 | 231.17 | -14.12 | 42.15 | 0.3498 | -737.0 | -654.8 | |
| 0.34 | 5.57 | 0.18 | 2.93 | 16.06 | 231.05 | -14.23 | 43.51 | 0.3447 | -918.0 | -768.5 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 17.13 | 230.17 | -15.12 | 43.03 | 0.3668 | -772.0 | -603.2 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 19.09 | 227.78 | -17.51 | 43.46 | 0.4151 | -646.0 | -523.5 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 17.36 | 227.86 | -17.43 | 46.52 | 0.3957 | -905.0 | -809.7 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 18.90 | 227.70 | -17.59 | 43.92 | 0.4139 | -770.0 | -702.7 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 19.21 | 227.47 | -17.82 | 43.73 | 0.4198 | -805.0 | -605.8 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 16.92 | 226.93 | -18.36 | 48.80 | 0.4023 | 998.0 | 824.3 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 15.69 | 226.62 | -18.66 | 51.71 | 0.3942 | 901.0 | 717.1 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 17.04 | 226.36 | -18.93 | 49.39 | 0.4103 | 1004.0 | 660.7 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 15.75 | 226.39 | -18.90 | 51.92 | 0.3977 | 887.0 | 699.1 | |
| 2.57 | 10.45 | 1.39 | 5.64 | 15.63 | 226.17 | -19.11 | 52.47 | 0.3993 | 1073.6 | 696.8 | |
| 5.82 | 57.28 | 3.16 | 31.10 | 15.99 | 225.65 | -19.64 | 52.45 | 0.4093 | 1279.0 | 645.4 | |
| 0.00 | 4.88 | 0.00 | 2.66 | 16.60 | 225.55 | -19.73 | 51.36 | 0.4161 | 925.0 | 641.4 | |
| 3.60 | -32.00 | 1.96 | -32.00 | 16.32 | 225.32 | -19.97 | 52.22 | 0.4164 | 853.1 | 999999 | |
| 11.56 | -32.00 | 6.28 | -32.00 | 15.83 | 225.31 | -19.98 | 53.22 | 0.4122 | 927.5 | 999999 | |
| 1.03 | -32.00 | 0.56 | -32.00 | 15.59 | 225.27 | -20.02 | 53.77 | 0.4106 | 819.3 | 999999 | |
| 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. | |