| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.18 | 209.07 | 18.79 | 108.67 | 9.01 | 357.08 | -14.87 | 56.74 | 0.3043 | -659.3 | -369.5 | |
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back to the solar disc SDO HMI 2011-12-12 16:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 0.65 | 9.79 | 2.55 | -9.40 | 41.90 | 0.2420 | -938.0 | -813.0 | |
| 1.87 | 185.65 | 0.97 | 96.38 | 9.20 | 357.99 | -13.96 | 54.63 | 0.2933 | -1142.5 | -447.2 | |
| 30.05 | -2.00 | 15.60 | -2.00 | 9.08 | 357.38 | -14.57 | 56.10 | 0.3006 | -1398.8 | 999999 | |
| 0.00 | 2.38 | 0.00 | 1.24 | 7.98 | 356.86 | -15.08 | 60.14 | 0.2984 | -869.0 | -680.9 | |
| 3.58 | -2.00 | 1.86 | -2.00 | 8.46 | 356.75 | -15.19 | 58.94 | 0.3040 | -977.4 | 999999 | |
| 0.00 | 2.64 | 0.00 | 1.37 | 8.82 | 356.40 | -15.55 | 58.50 | 0.3120 | -1017.0 | -722.6 | |
| 0.00 | 1.70 | 0.00 | 0.89 | 8.70 | 355.38 | -16.57 | 60.38 | 0.3257 | -838.0 | -605.5 | |
| 0.00 | 4.43 | 0.00 | 2.32 | 8.67 | 354.97 | -16.97 | 61.03 | 0.3313 | 703.0 | 627.9 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 9.48 | 354.90 | -17.04 | 59.01 | 0.3387 | -741.0 | -511.9 | |
| 0.68 | 2.81 | 0.36 | 1.48 | 8.70 | 354.63 | -17.32 | 61.42 | 0.3365 | 1077.4 | 832.5 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 8.91 | 354.56 | -17.39 | 60.97 | 0.3392 | 709.0 | 624.7 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 8.61 | 354.35 | -17.59 | 62.03 | 0.3399 | 803.0 | 582.8 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 9.60 | 353.83 | -18.12 | 60.18 | 0.3549 | 861.0 | 633.4 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 8.86 | 352.57 | -19.37 | 63.58 | 0.3675 | 918.0 | 702.7 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 10.45 | 351.14 | -20.81 | 61.44 | 0.3995 | 742.0 | 682.9 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 10.51 | 350.97 | -20.97 | 61.49 | 0.4022 | 671.0 | 612.1 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 6.61 | 347.98 | -23.96 | 72.95 | 0.4238 | 659.0 | 560.5 | |
| 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. | |