SDO HMI 2011-08-31 15:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.38 | 245.14 | 22.63 | 122.33 | 13.95 | 291.56 | 0.46 | 356.09 | 0.1198 | -565.5 | -349.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.83 | 0.00 | 2.45 | 18.72 | 293.65 | 2.55 | 348.13 | 0.2056 | 692.0 | 606.0 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 18.16 | 293.39 | 2.28 | 348.77 | 0.1954 | 902.0 | 740.4 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 18.04 | 293.32 | 2.22 | 348.96 | 0.1931 | 1074.0 | 844.4 | |
| 0.00 | 1.79 | 0.00 | 0.90 | 18.23 | 293.23 | 2.13 | 349.59 | 0.1960 | 938.0 | 685.0 | |
| 4.12 | 224.65 | 2.06 | 112.02 | 14.22 | 291.84 | 0.74 | 354.17 | 0.1239 | -1217.7 | -472.6 | |
| 14.86 | -5.00 | 7.40 | -5.00 | 13.39 | 291.81 | 0.71 | 353.68 | 0.1096 | -1351.7 | 999999 | |
| 26.40 | -5.00 | 13.17 | -5.00 | 13.82 | 291.59 | 0.49 | 355.90 | 0.1167 | -1282.0 | 999999 | |
| 0.00 | 1.88 | 0.00 | 0.94 | 13.00 | 289.54 | -1.56 | 14.63 | 0.1055 | 1059.0 | 745.5 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 11.20 | 289.12 | -1.98 | 25.70 | 0.0786 | 987.0 | 716.0 | |
| 0.00 | 2.60 | 0.00 | 1.30 | 15.21 | 287.42 | -3.68 | 23.83 | 0.1539 | 1031.0 | 842.4 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 15.00 | 287.30 | -3.80 | 25.13 | 0.1514 | 910.0 | 724.0 | |
| 0.00 | 2.15 | 0.00 | 1.08 | 16.43 | 286.83 | -4.27 | 23.88 | 0.1772 | 1025.0 | 769.9 | |
| 0.00 | 2.06 | 0.00 | 1.03 | 15.72 | 286.82 | -4.28 | 25.75 | 0.1663 | 983.0 | 674.6 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 16.49 | 286.64 | -4.46 | 24.67 | 0.1794 | 775.0 | 617.0 | |
| 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. | |