SDO HMI 2011-12-05 00:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.37 | 478.22 | 45.95 | 251.06 | 7.80 | 130.27 | 17.33 | 294.89 | 0.3255 | 6.6 | 70.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.68 | 0.00 | 0.37 | 7.67 | 137.49 | 24.55 | 287.09 | 0.4326 | -869.0 | -743.6 | |
| 0.00 | 2.30 | 0.00 | 1.26 | 7.88 | 137.47 | 24.53 | 287.57 | 0.4332 | -710.0 | -648.0 | |
| 20.39 | 117.24 | 11.03 | 63.49 | 6.66 | 135.90 | 22.96 | 285.72 | 0.4043 | -1227.1 | -371.4 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 6.81 | 135.07 | 22.13 | 286.62 | 0.3921 | -799.0 | -714.5 | |
| 0.00 | 3.24 | 0.00 | 1.75 | 7.26 | 135.06 | 22.12 | 287.73 | 0.3939 | -783.0 | -661.2 | |
| 0.00 | 3.16 | 0.00 | 1.70 | 6.75 | 134.81 | 21.87 | 286.65 | 0.3878 | -1077.0 | -798.0 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 5.95 | 134.52 | 21.58 | 284.81 | 0.3800 | -636.0 | -549.7 | |
| 0.00 | 2.56 | 0.00 | 1.37 | 6.93 | 134.47 | 21.53 | 287.34 | 0.3833 | -837.0 | -534.5 | |
| 8.02 | 45.56 | 4.29 | 24.33 | 6.57 | 134.42 | 21.48 | 286.47 | 0.3810 | -903.7 | -792.2 | |
| 1.28 | 3.58 | 0.69 | 1.92 | 7.94 | 134.49 | 21.55 | 289.84 | 0.3884 | 763.4 | 688.1 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 5.95 | 134.27 | 21.32 | 284.97 | 0.3760 | -765.0 | -500.4 | |
| 0.00 | 2.05 | 0.00 | 1.10 | 7.08 | 134.16 | 21.21 | 287.95 | 0.3791 | -689.0 | -578.9 | |
| 12.46 | -9.00 | 6.64 | -9.00 | 6.52 | 133.78 | 20.84 | 286.77 | 0.3707 | -1095.8 | 999999 | |
| 0.85 | 2.13 | 0.45 | 1.14 | 7.17 | 133.49 | 20.55 | 288.69 | 0.3693 | -973.8 | -870.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 5.15 | 133.03 | 20.09 | 283.60 | 0.3535 | -688.0 | -574.3 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 5.24 | 132.81 | 19.87 | 283.99 | 0.3503 | -1086.0 | -874.5 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 7.89 | 131.69 | 18.75 | 292.24 | 0.3455 | -864.0 | -703.2 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 7.21 | 131.44 | 18.50 | 290.61 | 0.3377 | -793.0 | -657.0 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 7.59 | 130.61 | 17.67 | 292.57 | 0.3272 | 827.0 | 662.6 | |
| 0.00 | 2.39 | 0.00 | 1.26 | 8.67 | 130.66 | 17.72 | 295.52 | 0.3348 | -925.0 | -723.5 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 10.82 | 130.68 | 17.74 | 301.13 | 0.3512 | -699.0 | -589.0 | |
| 0.00 | 2.47 | 0.00 | 1.28 | 7.15 | 128.94 | 16.00 | 293.22 | 0.2989 | -963.0 | -721.8 | |
| 0.00 | 2.05 | 0.00 | 1.07 | 8.46 | 128.84 | 15.90 | 297.33 | 0.3063 | 898.0 | 749.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 6.97 | 128.23 | 15.28 | 293.58 | 0.2868 | -859.0 | -613.4 | |
| 0.00 | 5.89 | 0.00 | 3.07 | 10.71 | 127.98 | 15.04 | 305.02 | 0.3127 | 669.0 | 690.9 | |
| 0.00 | 0.85 | 0.00 | 0.44 | 10.32 | 127.22 | 14.27 | 305.33 | 0.2987 | 1022.0 | 846.1 | |
| 0.00 | 2.13 | 0.00 | 1.11 | 10.53 | 127.17 | 14.22 | 306.01 | 0.2999 | 900.0 | 824.3 | |
| 41.90 | 254.02 | 21.58 | 130.86 | 8.53 | 126.74 | 13.80 | 300.88 | 0.2760 | 1314.0 | 421.6 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 11.25 | 126.70 | 13.76 | 308.85 | 0.3009 | 835.0 | 691.8 | |
| 0.00 | 2.39 | 0.00 | 1.24 | 11.07 | 126.66 | 13.72 | 308.45 | 0.2986 | 822.0 | 666.1 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 11.52 | 126.59 | 13.65 | 309.79 | 0.3023 | 664.0 | 557.7 | |
| 2.47 | -28.00 | 1.27 | -28.00 | 7.93 | 126.02 | 13.07 | 300.26 | 0.2605 | 1261.9 | 999999 | |
| 0.00 | 3.75 | 0.00 | 1.92 | 7.54 | 125.94 | 13.00 | 299.08 | 0.2563 | 800.0 | 646.4 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 11.19 | 125.74 | 12.80 | 310.70 | 0.2879 | 868.0 | 763.4 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 6.95 | 123.10 | 10.16 | 303.01 | 0.2097 | 977.0 | 773.5 | |
| 0.00 | 1.19 | 0.00 | 0.60 | 7.40 | 122.69 | 9.74 | 305.89 | 0.2081 | 877.0 | 649.0 | |
| 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. | |