SDO HMI 2011-05-31 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.01 | 99.92 | 16.69 | 61.62 | 15.77 | 40.67 | -32.97 | 61.56 | 0.5972 | -287.1 | -208.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.60 | 19.31 | 44.74 | -28.90 | 53.12 | 0.5723 | 617.0 | 546.7 | |
| 18.88 | 71.83 | 11.49 | 43.70 | 15.65 | 41.76 | -31.88 | 61.07 | 0.5833 | -1077.3 | -409.7 | |
| 0.00 | 1.26 | 0.00 | 0.78 | 15.44 | 40.52 | -33.12 | 62.22 | 0.5975 | -894.0 | -700.1 | |
| 2.98 | 4.79 | 1.84 | 2.95 | 15.15 | 40.53 | -33.11 | 62.65 | 0.5957 | -786.2 | -592.3 | |
| 0.00 | 1.54 | 0.00 | 0.96 | 16.46 | 39.68 | -33.96 | 61.20 | 0.6135 | -698.0 | -543.5 | |
| 0.00 | 2.53 | 0.00 | 1.59 | 15.29 | 38.76 | -34.88 | 63.52 | 0.6186 | 593.0 | 530.4 | |
| 0.00 | 1.45 | 0.00 | 0.92 | 16.82 | 38.21 | -35.43 | 61.58 | 0.6332 | 844.0 | 649.7 | |
| 0.00 | 1.45 | 0.00 | 0.91 | 14.98 | 38.59 | -35.06 | 64.09 | 0.6191 | 697.0 | 540.4 | |
| 1.99 | 2.80 | 1.26 | 1.77 | 15.39 | 38.47 | -35.17 | 63.54 | 0.6226 | 752.3 | 615.9 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 15.69 | 36.64 | -37.00 | 64.11 | 0.6462 | 675.0 | 529.1 | |
| 0.00 | 0.72 | 0.00 | 0.47 | 16.30 | 36.43 | -37.21 | 63.35 | 0.6517 | 641.0 | 576.5 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 15.67 | 36.25 | -37.39 | 64.35 | 0.6508 | 715.0 | 543.1 | |
| 0.00 | 1.08 | 0.00 | 0.71 | 15.92 | 36.08 | -37.56 | 64.08 | 0.6541 | 682.0 | 576.6 | |
| 3.16 | 7.32 | 2.10 | 4.85 | 16.85 | 35.30 | -38.34 | 63.17 | 0.6676 | 639.5 | 556.5 | |
| 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. | |