SDO HMI 2014-12-02 21:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.03 | 182.64 | 31.10 | 113.23 | -19.22 | 107.33 | 31.71 | 235.60 | 0.6032 | -63.5 | -6.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.02 | 4.01 | 0.67 | 2.63 | -19.92 | 111.68 | 36.06 | 237.71 | 0.6570 | 686.0 | 553.7 | |
| 0.00 | 1.45 | 0.00 | 0.94 | -20.07 | 110.75 | 35.13 | 236.90 | 0.6475 | 653.0 | 513.9 | |
| 9.14 | 19.47 | 5.89 | 12.55 | -19.59 | 110.59 | 34.97 | 237.46 | 0.6429 | 847.6 | 578.6 | |
| 0.00 | 2.56 | 0.00 | 1.64 | -19.56 | 110.28 | 34.66 | 237.30 | 0.6391 | 954.0 | 851.1 | |
| 2.31 | 4.78 | 1.47 | 3.06 | -19.02 | 110.07 | 34.45 | 237.92 | 0.6335 | 902.1 | 657.8 | |
| 0.51 | 2.99 | 0.33 | 1.92 | -20.06 | 110.21 | 34.59 | 236.55 | 0.6415 | 742.3 | 686.8 | |
| 0.00 | 1.45 | 0.00 | 0.92 | -19.05 | 109.85 | 34.23 | 237.73 | 0.6312 | 580.0 | 544.7 | |
| 1.11 | 21.09 | 0.71 | 13.33 | -19.02 | 109.66 | 34.03 | 237.64 | 0.6287 | 634.5 | 609.7 | |
| 1.79 | -8.00 | 1.13 | -8.00 | -18.83 | 109.42 | 33.80 | 237.76 | 0.6249 | 797.9 | 999999 | |
| 1.45 | -8.00 | 0.92 | -8.00 | -19.02 | 109.32 | 33.69 | 237.41 | 0.6248 | 882.4 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.06 | -17.76 | 108.30 | 32.67 | 238.54 | 0.6050 | -689.0 | -542.1 | |
| 0.00 | 0.77 | 0.00 | 0.49 | -20.50 | 108.91 | 33.29 | 235.04 | 0.6297 | 603.0 | 522.3 | |
| 1.62 | 4.10 | 1.01 | 2.56 | -18.73 | 108.46 | 32.84 | 237.24 | 0.6131 | -385.1 | -189.6 | |
| 0.00 | 1.11 | 0.00 | 0.69 | -18.51 | 108.23 | 32.61 | 237.39 | 0.6090 | 382.0 | 405.2 | |
| 0.00 | 0.77 | 0.00 | 0.49 | -20.24 | 108.51 | 32.89 | 235.11 | 0.6235 | 750.0 | 563.9 | |
| 0.00 | 1.02 | 0.00 | 0.65 | -20.46 | 108.53 | 32.90 | 234.81 | 0.6251 | 733.0 | 625.2 | |
| 6.66 | 11.10 | 4.13 | 6.89 | -18.69 | 107.79 | 32.17 | 236.80 | 0.6050 | -603.1 | -204.9 | |
| 1.02 | 2.13 | 0.63 | 1.32 | -18.13 | 107.67 | 32.05 | 237.54 | 0.5999 | 750.0 | 653.6 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -18.50 | 107.31 | 31.69 | 236.72 | 0.5981 | -403.0 | -249.8 | |
| 0.00 | 1.20 | 0.00 | 0.73 | -17.65 | 107.03 | 31.41 | 237.78 | 0.5892 | -634.0 | -427.3 | |
| 4.27 | 5.81 | 2.60 | 3.54 | -17.37 | 106.87 | 31.24 | 238.08 | 0.5854 | 780.7 | 488.4 | |
| 0.00 | 1.62 | 0.00 | 0.99 | -17.68 | 106.74 | 31.12 | 237.52 | 0.5860 | -99.0 | -94.8 | |
| 0.43 | 2.65 | 0.26 | 1.63 | -19.18 | 106.79 | 31.17 | 235.32 | 0.5967 | -693.4 | -502.4 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -19.18 | 106.50 | 30.88 | 235.09 | 0.5933 | -608.0 | -579.3 | |
| 0.00 | 4.61 | 0.00 | 2.83 | -18.99 | 106.42 | 30.80 | 235.31 | 0.5911 | -818.0 | -626.3 | |
| 0.00 | 1.54 | 0.00 | 0.94 | -18.40 | 106.23 | 30.61 | 236.04 | 0.5847 | -337.0 | -397.8 | |
| 0.43 | 1.11 | 0.26 | 0.67 | -18.77 | 105.80 | 30.17 | 235.14 | 0.5822 | -881.4 | -836.0 | |
| 0.00 | 1.20 | 0.00 | 0.73 | -18.96 | 105.83 | 30.21 | 234.89 | 0.5840 | -836.0 | -638.6 | |
| 0.00 | 0.94 | 0.00 | 0.57 | -19.11 | 105.79 | 30.17 | 234.62 | 0.5847 | -781.0 | -616.4 | |
| 0.00 | 2.90 | 0.00 | 1.77 | -19.30 | 105.76 | 30.14 | 234.32 | 0.5856 | -754.0 | -627.1 | |
| 2.73 | 68.30 | 1.66 | 41.52 | -19.33 | 105.33 | 29.71 | 233.92 | 0.5809 | -977.9 | -385.3 | |
| 13.06 | -31.00 | 7.94 | -31.00 | -19.64 | 105.25 | 29.63 | 233.39 | 0.5823 | -1021.5 | 999999 | |
| 1.88 | 4.95 | 1.13 | 2.98 | -18.67 | 104.77 | 29.15 | 234.44 | 0.5695 | 753.0 | 585.9 | |
| 0.00 | 1.37 | 0.00 | 0.82 | -18.48 | 104.41 | 28.79 | 234.42 | 0.5639 | 744.0 | 678.0 | |
| 0.00 | 1.11 | 0.00 | 0.67 | -19.57 | 103.80 | 28.18 | 232.22 | 0.5651 | -771.0 | -622.9 | |
| 0.60 | 1.62 | 0.36 | 0.96 | -18.84 | 103.38 | 27.76 | 232.93 | 0.5546 | -581.7 | -507.2 | |
| 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. | |