SDO HMI 2011-01-05 17:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.71 | 95.49 | 13.02 | 49.98 | -14.42 | 208.01 | 15.20 | 232.23 | 0.3204 | -187.1 | -172.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.10 | 0.00 | 0.59 | -12.22 | 212.08 | 19.27 | 244.37 | 0.3593 | 852.0 | 698.6 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -16.42 | 212.10 | 19.29 | 234.42 | 0.3913 | 661.0 | 584.5 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -15.61 | 211.99 | 19.18 | 236.07 | 0.3830 | 541.0 | 391.8 | |
| 2.80 | 20.55 | 1.50 | 10.97 | -15.16 | 211.75 | 18.94 | 236.79 | 0.3761 | 984.0 | 744.7 | |
| 4.08 | -4.00 | 2.17 | -4.00 | -14.74 | 211.72 | 18.90 | 237.72 | 0.3722 | 828.1 | 999999 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -15.97 | 211.80 | 18.98 | 235.00 | 0.3835 | 784.0 | 570.0 | |
| 8.83 | 15.37 | 4.69 | 8.16 | -14.48 | 211.18 | 18.36 | 237.64 | 0.3627 | 1045.2 | 863.4 | |
| 1.53 | -7.00 | 0.81 | -7.00 | -14.57 | 210.90 | 18.08 | 237.04 | 0.3596 | 966.6 | 999999 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -12.40 | 210.28 | 17.47 | 241.79 | 0.3342 | 714.0 | 554.3 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -14.62 | 210.26 | 17.45 | 236.05 | 0.3513 | 850.0 | 666.1 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -13.78 | 209.94 | 17.13 | 237.68 | 0.3399 | 889.0 | 742.8 | |
| 0.00 | 0.93 | 0.00 | 0.50 | -16.25 | 209.99 | 17.17 | 231.79 | 0.3623 | 726.0 | 673.7 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -13.97 | 207.30 | 14.49 | 232.92 | 0.3057 | -806.0 | -642.2 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -13.83 | 206.82 | 14.01 | 232.42 | 0.2980 | -953.0 | -689.0 | |
| 0.00 | 2.46 | 0.00 | 1.27 | -13.54 | 206.06 | 13.24 | 231.72 | 0.2850 | -659.0 | -376.8 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -15.22 | 206.13 | 13.32 | 227.37 | 0.3034 | -812.0 | -668.5 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -14.32 | 205.92 | 13.10 | 229.27 | 0.2912 | -814.0 | -680.3 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -13.91 | 205.74 | 12.92 | 230.03 | 0.2845 | -824.0 | -626.4 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -14.12 | 205.66 | 12.84 | 229.28 | 0.2857 | -758.0 | -605.2 | |
| 0.00 | 2.29 | 0.00 | 1.19 | -14.57 | 205.62 | 12.80 | 227.98 | 0.2900 | -871.0 | -750.0 | |
| 0.00 | 2.21 | 0.00 | 1.14 | -14.30 | 205.60 | 12.79 | 228.67 | 0.2869 | -818.0 | -723.2 | |
| 0.00 | 3.14 | 0.00 | 1.62 | -13.73 | 205.42 | 12.60 | 229.84 | 0.2786 | -755.0 | -663.3 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -14.54 | 205.43 | 12.62 | 227.65 | 0.2874 | -845.0 | -716.0 | |
| 0.85 | 4.50 | 0.44 | 2.32 | -14.21 | 205.26 | 12.44 | 228.15 | 0.2817 | -1082.4 | -911.1 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -14.48 | 205.08 | 12.27 | 227.02 | 0.2825 | -868.0 | -761.4 | |
| 0.00 | 4.25 | 0.00 | 2.19 | -13.86 | 205.02 | 12.20 | 228.61 | 0.2748 | -1120.0 | -979.8 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -14.16 | 204.94 | 12.13 | 227.59 | 0.2771 | -928.0 | -766.5 | |
| 2.46 | 4.67 | 1.27 | 2.41 | -14.46 | 204.80 | 11.99 | 226.45 | 0.2788 | -1082.4 | -826.8 | |
| 0.00 | 3.99 | 0.00 | 2.05 | -14.10 | 204.54 | 11.72 | 226.80 | 0.2715 | -1094.0 | -890.6 | |
| 4.16 | 4.76 | 2.14 | 2.44 | -13.47 | 204.47 | 11.66 | 228.44 | 0.2638 | -1028.2 | -792.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -13.77 | 204.30 | 11.49 | 227.16 | 0.2650 | -895.0 | -769.8 | |
| 0.00 | 1.95 | 0.00 | 1.00 | -14.11 | 204.07 | 11.26 | 225.66 | 0.2659 | -920.0 | -822.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -15.19 | 204.13 | 11.31 | 222.93 | 0.2792 | -716.0 | -600.6 | |
| 0.00 | 1.95 | 0.00 | 1.00 | -14.02 | 203.66 | 10.85 | 224.87 | 0.2601 | -761.0 | -582.7 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -16.62 | 202.65 | 9.83 | 215.70 | 0.2817 | -769.0 | -668.5 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -14.47 | 201.22 | 8.40 | 216.58 | 0.2385 | -904.0 | -676.8 | |
| 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. | |