SDO HMI 2011-12-16 07:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.41 | 108.79 | 11.77 | 65.46 | 8.36 | 357.47 | 33.29 | 286.47 | 0.5682 | -262.8 | -212.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.41 | 90.82 | 11.77 | 55.12 | 8.31 | 358.26 | 34.08 | 286.03 | 0.5791 | -1137.8 | -369.7 | |
| 0.00 | 1.70 | 0.00 | 1.03 | 11.03 | 356.91 | 32.74 | 291.22 | 0.5716 | -774.0 | -599.0 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 11.08 | 355.57 | 31.39 | 292.06 | 0.5537 | -620.0 | -518.3 | |
| 0.00 | 2.38 | 0.00 | 1.39 | 9.29 | 354.64 | 30.46 | 289.46 | 0.5328 | 668.0 | 573.8 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 9.62 | 354.08 | 29.90 | 290.36 | 0.5264 | 599.0 | 541.2 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 9.53 | 353.93 | 29.76 | 290.28 | 0.5239 | 760.0 | 632.5 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 9.74 | 353.78 | 29.61 | 290.75 | 0.5228 | 698.0 | 546.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 8.09 | 353.57 | 29.39 | 287.82 | 0.5124 | 630.0 | 592.1 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 9.46 | 353.62 | 29.44 | 290.35 | 0.5192 | 868.0 | 781.9 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 8.13 | 352.28 | 28.10 | 288.63 | 0.4941 | 741.0 | 569.2 | |
| 0.00 | 1.96 | 0.00 | 1.12 | 9.15 | 352.26 | 28.08 | 290.60 | 0.4985 | 871.0 | 704.2 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 8.01 | 351.80 | 27.62 | 288.67 | 0.4866 | 883.0 | 776.5 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 6.22 | 351.14 | 26.97 | 285.40 | 0.4695 | 777.0 | 561.5 | |
| 0.00 | 3.06 | 0.00 | 1.70 | 5.20 | 350.36 | 26.18 | 283.65 | 0.4541 | 781.0 | 640.2 | |
| 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. | |