| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.50 | 327.82 | 30.44 | 173.47 | 17.57 | 223.34 | -13.19 | 38.28 | 0.3528 | -737.0 | -349.6 | |
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back to the solar disc SDO HMI 2011-11-25 15:58:57 UT
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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 | 0.63 | 18.85 | 225.38 | -11.15 | 31.66 | 0.3502 | 991.0 | 791.3 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 19.03 | 225.08 | -11.45 | 32.04 | 0.3553 | 935.0 | 747.4 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 18.85 | 224.93 | -11.60 | 32.66 | 0.3541 | 724.0 | 558.5 | |
| 0.00 | 7.87 | 0.00 | 4.18 | 19.25 | 224.74 | -11.79 | 32.43 | 0.3611 | 761.0 | 723.6 | |
| 14.03 | 261.75 | 7.39 | 138.30 | 17.17 | 223.87 | -12.66 | 37.90 | 0.3423 | -1334.0 | -431.5 | |
| 3.34 | 4.88 | 1.78 | 2.60 | 19.37 | 223.67 | -12.85 | 34.48 | 0.3723 | -1034.0 | -890.8 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 19.61 | 223.27 | -13.26 | 34.90 | 0.3793 | -680.0 | -472.7 | |
| 26.53 | -5.00 | 14.03 | -5.00 | 17.57 | 223.33 | -13.19 | 38.29 | 0.3527 | -1311.5 | 999999 | |
| 0.60 | 2.05 | 0.32 | 1.10 | 19.74 | 223.09 | -13.43 | 35.04 | 0.3824 | -742.1 | -737.1 | |
| 1.11 | 1.28 | 0.59 | 0.68 | 16.52 | 222.42 | -14.10 | 42.15 | 0.3496 | -666.6 | -668.5 | |
| 11.89 | 37.14 | 6.33 | 19.80 | 17.81 | 222.16 | -14.36 | 40.18 | 0.3677 | -983.5 | -276.1 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 16.00 | 221.44 | -15.08 | 45.10 | 0.3547 | 949.0 | 704.4 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 15.48 | 221.48 | -15.04 | 46.12 | 0.3485 | 858.0 | 634.7 | |
| 0.00 | 2.91 | 0.00 | 1.55 | 17.50 | 221.29 | -15.24 | 42.39 | 0.3734 | -727.0 | -575.7 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 16.24 | 220.98 | -15.55 | 45.44 | 0.3628 | 943.0 | 781.9 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 16.60 | 220.43 | -16.09 | 45.66 | 0.3730 | 852.0 | 651.6 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 18.44 | 219.52 | -17.01 | 43.68 | 0.4036 | 812.0 | 691.9 | |
| 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. | |