SDO HMI 2011-11-26 00:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.75 | 41.08 | 19.85 | 51.41 | 16.82 | 297.57 | 66.02 | 287.70 | 0.9187 | -7.9 | 114.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.73 | 12.75 | 8.18 | 18.29 | 16.45 | 300.82 | 69.26 | 286.97 | 0.9393 | -414.9 | -32.4 | |
| 0.00 | 0.77 | 0.00 | 1.07 | 15.79 | 300.31 | 68.75 | 286.31 | 0.9360 | -304.0 | -240.6 | |
| 1.03 | 1.97 | 1.43 | 2.75 | 16.00 | 300.38 | 68.83 | 286.53 | 0.9366 | -316.8 | -282.5 | |
| 0.00 | 1.03 | 0.00 | 1.27 | 16.32 | 297.44 | 65.89 | 287.13 | 0.9184 | -411.0 | -380.2 | |
| 0.00 | 0.86 | 0.00 | 1.05 | 17.03 | 297.16 | 65.61 | 287.94 | 0.9170 | -418.0 | -361.8 | |
| 0.00 | 1.03 | 0.00 | 1.19 | 16.27 | 295.50 | 63.95 | 287.29 | 0.9051 | -268.0 | -201.2 | |
| 1.11 | 1.80 | 1.27 | 2.05 | 16.15 | 295.22 | 63.67 | 287.20 | 0.9030 | 159.8 | 85.0 | |
| 1.03 | 2.05 | 1.18 | 2.36 | 16.61 | 295.36 | 63.80 | 287.69 | 0.9043 | 245.1 | 61.3 | |
| 0.51 | 2.05 | 0.58 | 2.33 | 16.34 | 294.98 | 63.43 | 287.43 | 0.9014 | 354.8 | 279.8 | |
| 3.17 | 4.79 | 3.64 | 5.50 | 17.39 | 295.21 | 63.65 | 288.56 | 0.9039 | 385.6 | 255.4 | |
| 0.00 | 0.68 | 0.00 | 0.77 | 17.12 | 294.76 | 63.20 | 288.32 | 0.9005 | 343.0 | 341.0 | |
| 0.00 | 4.11 | 0.00 | 4.68 | 17.89 | 294.97 | 63.41 | 289.14 | 0.9027 | 574.0 | 433.4 | |
| 3.17 | 7.19 | 3.57 | 8.10 | 17.56 | 294.68 | 63.13 | 288.81 | 0.9003 | 567.5 | 499.6 | |
| 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. | |