| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.86 | 51.00 | 23.94 | 60.86 | 16.72 | 297.42 | 64.76 | 287.72 | 0.9102 | -34.0 | -2.0 | |
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back to the solar disc SDO HMI 2011-11-25 22:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.22 | 14.55 | 11.13 | 19.80 | 16.42 | 300.76 | 68.11 | 287.04 | 0.9325 | -422.4 | -34.9 | |
| 0.00 | 2.65 | 0.00 | 3.51 | 15.85 | 300.27 | 67.61 | 286.46 | 0.9291 | -523.0 | -307.1 | |
| 0.00 | 2.48 | 0.00 | 3.00 | 16.03 | 297.90 | 65.24 | 286.88 | 0.9138 | -344.0 | -199.4 | |
| 0.00 | 1.03 | 0.00 | 1.21 | 16.48 | 297.22 | 64.56 | 287.45 | 0.9095 | -462.0 | -421.1 | |
| 0.00 | 1.03 | 0.00 | 1.21 | 17.00 | 297.19 | 64.54 | 288.02 | 0.9097 | -482.0 | -451.6 | |
| 0.00 | 0.94 | 0.00 | 1.06 | 14.94 | 295.98 | 63.32 | 285.89 | 0.8995 | -390.0 | -290.5 | |
| 1.11 | 1.88 | 1.23 | 2.08 | 16.15 | 295.35 | 62.69 | 287.30 | 0.8958 | 121.3 | 58.8 | |
| 0.94 | 2.31 | 1.05 | 2.57 | 16.61 | 295.47 | 62.82 | 287.80 | 0.8971 | 295.7 | 103.1 | |
| 1.37 | 2.31 | 1.51 | 2.54 | 16.34 | 295.18 | 62.52 | 287.53 | 0.8947 | 309.4 | 209.9 | |
| 2.74 | 5.13 | 3.03 | 5.70 | 17.39 | 295.26 | 62.60 | 288.69 | 0.8963 | 396.9 | 142.8 | |
| 0.00 | 1.20 | 0.00 | 1.34 | 17.66 | 295.43 | 62.77 | 288.97 | 0.8978 | 241.0 | 152.7 | |
| 0.00 | 2.14 | 0.00 | 2.34 | 16.81 | 294.91 | 62.26 | 288.09 | 0.8932 | 471.0 | 361.1 | |
| 0.00 | 1.20 | 0.00 | 1.31 | 17.06 | 294.86 | 62.20 | 288.37 | 0.8930 | 500.0 | 362.4 | |
| 2.40 | 3.59 | 2.64 | 3.95 | 17.83 | 294.99 | 62.33 | 289.21 | 0.8947 | 458.6 | 417.9 | |
| 3.08 | 5.73 | 3.35 | 6.23 | 17.46 | 294.70 | 62.04 | 288.85 | 0.8922 | 598.4 | 503.9 | |
| 0.00 | 1.20 | 0.00 | 1.28 | 16.83 | 294.19 | 61.54 | 288.20 | 0.8878 | -337.0 | -282.6 | |
| 0.00 | 1.63 | 0.00 | 1.73 | 17.05 | 294.06 | 61.40 | 288.47 | 0.8869 | -471.0 | -402.6 | |
| 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. | |