SDO HMI 2011-08-28 00:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.58 | 32.83 | 5.27 | 16.38 | 7.46 | 345.19 | 6.22 | 272.01 | 0.1083 | -144.4 | -83.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.43 | 0.00 | 0.73 | 7.24 | 351.70 | 12.72 | 271.35 | 0.2195 | -885.0 | -754.4 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 8.39 | 350.42 | 11.45 | 277.17 | 0.1988 | -872.0 | -675.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.12 | 350.32 | 11.34 | 275.85 | 0.1966 | -903.0 | -664.5 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 7.70 | 350.15 | 11.18 | 273.74 | 0.1934 | -945.0 | -729.9 | |
| 0.00 | 2.15 | 0.00 | 1.09 | 7.94 | 350.09 | 11.12 | 275.02 | 0.1926 | -1021.0 | -742.8 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 7.07 | 346.70 | 7.73 | 270.17 | 0.1340 | -877.0 | -701.7 | |
| 0.00 | 1.70 | 0.00 | 0.85 | 8.15 | 345.73 | 6.76 | 279.20 | 0.1186 | -1093.0 | -881.0 | |
| 2.96 | 4.04 | 1.48 | 2.01 | 8.39 | 345.70 | 6.73 | 281.27 | 0.1188 | -1126.2 | -849.1 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 7.97 | 345.67 | 6.69 | 277.75 | 0.1171 | -926.0 | -737.2 | |
| 0.00 | 1.88 | 0.00 | 0.94 | 7.72 | 343.21 | 4.24 | 278.51 | 0.0743 | 1050.0 | 792.9 | |
| 2.69 | 4.04 | 1.34 | 2.00 | 7.12 | 343.02 | 4.05 | 270.32 | 0.0703 | 1086.9 | 793.4 | |
| 4.93 | 9.15 | 2.45 | 4.54 | 6.73 | 342.43 | 3.46 | 263.83 | 0.0606 | 1065.2 | 829.3 | |
| 0.00 | 1.26 | 0.00 | 0.62 | 7.19 | 341.77 | 2.79 | 271.71 | 0.0486 | 905.0 | 663.7 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 6.98 | 341.61 | 2.64 | 267.18 | 0.0460 | 818.0 | 580.2 | |
| 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. | |