SDO HMI 2011-08-26 03:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.70 | 47.68 | 8.79 | 24.87 | 7.57 | 345.62 | -18.13 | 87.37 | 0.3098 | -31.8 | -103.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.63 | 6.92 | 352.37 | -11.38 | 90.03 | 0.1968 | -886.0 | -607.3 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 6.56 | 352.34 | -11.41 | 91.88 | 0.1975 | -900.0 | -724.8 | |
| 0.00 | 2.96 | 0.00 | 1.50 | 6.99 | 351.33 | -12.41 | 89.60 | 0.2144 | -952.0 | -842.2 | |
| 0.00 | 1.53 | 0.00 | 0.77 | 7.35 | 351.29 | -12.46 | 87.90 | 0.2150 | -971.0 | -844.1 | |
| 0.00 | 2.15 | 0.00 | 1.10 | 8.01 | 349.83 | -13.92 | 85.20 | 0.2402 | -813.0 | -666.6 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 7.12 | 348.72 | -15.03 | 88.84 | 0.2585 | -1057.0 | -888.6 | |
| 0.00 | 2.15 | 0.00 | 1.11 | 6.59 | 348.26 | -15.49 | 90.82 | 0.2664 | -1087.0 | -843.5 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 6.92 | 347.90 | -15.84 | 89.57 | 0.2723 | -719.0 | -516.1 | |
| 1.71 | 7.36 | 0.89 | 3.84 | 7.87 | 345.63 | -18.12 | 86.29 | 0.3101 | -1041.3 | -882.7 | |
| 2.96 | -9.00 | 1.54 | -9.00 | 7.65 | 345.58 | -18.17 | 86.98 | 0.3109 | -893.5 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 9.95 | 344.65 | -19.10 | 79.97 | 0.3288 | 826.0 | 602.1 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 7.72 | 343.63 | -20.12 | 86.82 | 0.3429 | 812.0 | 699.0 | |
| 12.03 | 21.91 | 6.36 | 11.57 | 7.71 | 343.24 | -20.51 | 86.88 | 0.3492 | 1054.2 | 683.1 | |
| 0.00 | 2.51 | 0.00 | 1.33 | 7.63 | 342.88 | -20.87 | 87.10 | 0.3550 | 715.0 | 584.7 | |
| 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. | |