SDO HMI 2011-07-01 13:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.98 | 41.41 | 7.14 | 21.18 | 15.96 | 23.73 | 4.80 | 339.86 | 0.2461 | 57.8 | -148.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.54 | 10.44 | 2.82 | 5.31 | 13.46 | 26.67 | 7.74 | 324.57 | 0.2269 | 1099.0 | 750.6 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 15.27 | 25.30 | 6.37 | 333.53 | 0.2411 | -905.0 | -614.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 15.65 | 25.22 | 6.28 | 334.53 | 0.2462 | -1008.0 | -805.5 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 16.09 | 25.17 | 6.23 | 335.48 | 0.2525 | -696.0 | -531.5 | |
| 1.09 | 3.91 | 0.56 | 2.00 | 16.34 | 25.02 | 6.08 | 336.42 | 0.2553 | -983.5 | -691.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.81 | 25.00 | 6.07 | 335.58 | 0.2470 | -775.0 | -631.7 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 15.53 | 24.55 | 5.61 | 336.73 | 0.2396 | -1168.0 | -930.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.59 | 24.40 | 5.46 | 335.61 | 0.2241 | -892.0 | -766.1 | |
| 0.00 | 2.63 | 0.00 | 1.35 | 16.53 | 23.59 | 4.65 | 341.78 | 0.2498 | -1034.0 | -815.1 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 18.33 | 21.38 | 2.45 | 351.35 | 0.2707 | -822.0 | -627.0 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 17.92 | 21.22 | 2.28 | 351.70 | 0.2635 | 433.0 | 379.9 | |
| 1.45 | 2.72 | 0.74 | 1.40 | 17.48 | 21.08 | 2.15 | 351.93 | 0.2558 | 777.6 | 449.9 | |
| 5.90 | 6.54 | 3.02 | 3.35 | 17.23 | 20.79 | 1.86 | 352.88 | 0.2509 | 1082.0 | 909.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.77 | 20.57 | 1.64 | 353.95 | 0.2595 | 787.0 | 521.1 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 18.15 | 20.35 | 1.42 | 354.90 | 0.2655 | 737.0 | 601.6 | |
| 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. | |