SDO HMI 2011-05-27 04:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.05 | 106.17 | 27.86 | 56.80 | 20.54 | 130.24 | 3.13 | 352.32 | 0.3779 | -125.0 | 108.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.63 | 20.75 | 134.61 | 7.49 | 342.00 | 0.3961 | 650.0 | 500.1 | |
| 25.35 | 47.01 | 13.63 | 25.25 | 20.98 | 132.16 | 5.05 | 347.77 | 0.3893 | -1046.9 | -564.1 | |
| 4.42 | -2.00 | 2.37 | -2.00 | 20.65 | 131.63 | 4.51 | 348.84 | 0.3823 | -1053.3 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 20.38 | 131.46 | 4.34 | 349.12 | 0.3776 | -749.0 | -613.3 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 21.37 | 130.61 | 3.49 | 351.63 | 0.3910 | -900.0 | -688.8 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 19.96 | 130.15 | 3.04 | 352.17 | 0.3673 | 650.0 | 499.8 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 21.40 | 130.15 | 3.03 | 352.72 | 0.3905 | -275.0 | -375.3 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 21.23 | 129.27 | 2.15 | 354.79 | 0.3863 | -840.0 | -622.8 | |
| 1.44 | 10.01 | 0.77 | 5.35 | 20.48 | 128.96 | 1.85 | 355.35 | 0.3737 | 755.4 | 580.1 | |
| 0.00 | 2.71 | 0.00 | 1.44 | 19.83 | 128.96 | 1.84 | 355.21 | 0.3630 | 635.0 | 624.3 | |
| 2.98 | 3.61 | 1.58 | 1.91 | 19.50 | 128.79 | 1.67 | 355.56 | 0.3575 | 1049.7 | 877.4 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 19.66 | 128.57 | 1.45 | 356.19 | 0.3599 | 910.0 | 692.7 | |
| 17.86 | 33.20 | 9.51 | 17.68 | 20.09 | 128.12 | 1.00 | 357.42 | 0.3664 | 1047.5 | 644.8 | |
| 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. | |