SDO HMI 2011-05-31 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.15 | 39.46 | 21.22 | 44.73 | 21.57 | 131.88 | 61.53 | 294.57 | 0.9001 | -249.2 | -18.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 19.60 | 1.52 | 23.33 | 22.31 | 133.45 | 63.10 | 295.03 | 0.9123 | 201.4 | 65.0 | |
| 11.02 | -1.00 | 13.06 | -1.00 | 22.18 | 133.12 | 62.77 | 294.95 | 0.9099 | -505.6 | 999999 | |
| 2.08 | 3.61 | 2.33 | 4.06 | 20.81 | 131.82 | 61.47 | 293.75 | 0.8990 | -332.3 | -368.6 | |
| 0.00 | 1.90 | 0.00 | 2.10 | 20.58 | 131.38 | 61.03 | 293.58 | 0.8955 | -604.0 | -497.0 | |
| 3.79 | 4.97 | 4.31 | 5.64 | 21.60 | 132.04 | 61.69 | 294.56 | 0.9018 | -355.8 | -310.2 | |
| 0.00 | 2.26 | 0.00 | 2.51 | 21.10 | 131.48 | 61.12 | 294.14 | 0.8970 | -513.0 | -363.6 | |
| 0.00 | 0.81 | 0.00 | 0.88 | 20.73 | 130.82 | 60.46 | 293.88 | 0.8917 | -620.0 | -545.1 | |
| 0.00 | 0.99 | 0.00 | 1.00 | 19.11 | 128.54 | 58.19 | 292.59 | 0.8716 | 597.0 | 497.2 | |
| 0.00 | 0.90 | 0.00 | 0.90 | 19.59 | 128.20 | 57.85 | 293.21 | 0.8698 | 314.0 | 335.1 | |
| 0.00 | 1.08 | 0.00 | 1.07 | 20.17 | 127.62 | 57.27 | 294.00 | 0.8664 | 297.0 | 222.8 | |
| 0.00 | 0.90 | 0.00 | 0.87 | 20.13 | 127.00 | 56.65 | 294.12 | 0.8613 | 536.0 | 460.4 | |
| 0.00 | 0.99 | 0.00 | 0.95 | 20.25 | 126.36 | 56.01 | 294.42 | 0.8563 | 545.0 | 490.7 | |
| 0.00 | 1.45 | 0.00 | 1.42 | 22.03 | 127.11 | 56.75 | 296.23 | 0.8662 | 523.0 | 412.6 | |
| 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. | |