SDO HMI 2011-01-05 14:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.80 | 101.65 | 10.87 | 52.95 | -14.47 | 208.55 | 14.08 | 230.05 | 0.3062 | -137.9 | -33.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.23 | 0.00 | 1.72 | -16.35 | 212.07 | 17.60 | 232.19 | 0.3689 | 601.0 | 541.9 | |
| 3.91 | 23.36 | 2.07 | 12.35 | -15.12 | 211.67 | 17.20 | 234.45 | 0.3525 | 968.0 | 654.2 | |
| 9.68 | 19.19 | 5.09 | 10.10 | -14.38 | 211.10 | 16.63 | 235.41 | 0.3383 | 1063.3 | 818.2 | |
| 1.44 | -3.00 | 0.76 | -3.00 | -14.47 | 210.89 | 16.42 | 234.85 | 0.3362 | 991.7 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -15.86 | 210.90 | 16.43 | 231.51 | 0.3492 | 808.0 | 584.6 | |
| 0.00 | 2.72 | 0.00 | 1.42 | -14.06 | 210.42 | 15.94 | 235.15 | 0.3261 | 888.0 | 717.3 | |
| 0.00 | 1.78 | 0.00 | 0.93 | -14.57 | 210.20 | 15.73 | 233.48 | 0.3279 | 951.0 | 713.0 | |
| 0.00 | 2.55 | 0.00 | 1.33 | -13.86 | 209.96 | 15.49 | 234.94 | 0.3182 | 853.0 | 726.6 | |
| 0.00 | 1.87 | 0.00 | 0.97 | -13.14 | 208.22 | 13.75 | 233.86 | 0.2880 | 663.0 | 494.5 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -13.95 | 207.49 | 13.02 | 230.08 | 0.2864 | -652.0 | -576.7 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -13.90 | 207.27 | 12.80 | 229.77 | 0.2829 | -800.0 | -638.1 | |
| 0.00 | 2.89 | 0.00 | 1.49 | -13.75 | 206.73 | 12.26 | 229.00 | 0.2746 | -849.0 | -618.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -14.21 | 205.98 | 11.51 | 225.96 | 0.2703 | -957.0 | -745.6 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -13.62 | 205.83 | 11.36 | 227.27 | 0.2617 | -776.0 | -590.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -14.78 | 205.86 | 11.39 | 224.12 | 0.2754 | -852.0 | -733.0 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -14.28 | 205.61 | 11.14 | 224.88 | 0.2666 | -783.0 | -601.6 | |
| 0.00 | 1.87 | 0.00 | 0.96 | -14.46 | 205.56 | 11.09 | 224.25 | 0.2681 | -923.0 | -837.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -13.71 | 205.49 | 11.02 | 226.17 | 0.2586 | -782.0 | -661.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -14.55 | 205.38 | 10.91 | 223.54 | 0.2671 | -876.0 | -720.9 | |
| 0.00 | 5.86 | 0.00 | 3.01 | -14.34 | 205.21 | 10.74 | 223.68 | 0.2627 | -786.0 | -880.2 | |
| 0.00 | 6.11 | 0.00 | 3.13 | -13.86 | 205.10 | 10.63 | 224.71 | 0.2557 | -834.0 | -880.2 | |
| 2.63 | 6.88 | 1.35 | 3.53 | -14.41 | 204.78 | 10.31 | 222.36 | 0.2585 | -1142.6 | -753.0 | |
| 3.14 | 3.57 | 1.60 | 1.82 | -13.45 | 204.52 | 10.05 | 224.35 | 0.2440 | -1082.5 | -904.8 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -14.35 | 204.53 | 10.06 | 221.83 | 0.2550 | -925.0 | -742.5 | |
| 0.00 | 3.74 | 0.00 | 1.91 | -14.14 | 204.49 | 10.02 | 222.29 | 0.2519 | -1160.0 | -896.7 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -13.75 | 204.32 | 9.85 | 222.90 | 0.2452 | -1103.0 | -834.2 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -14.05 | 204.09 | 9.62 | 221.38 | 0.2463 | -1135.0 | -903.4 | |
| 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. | |