SDO HMI 2011-09-01 18:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.68 | 169.92 | 18.96 | 87.67 | 13.60 | 291.52 | 15.29 | 294.43 | 0.2830 | -672.3 | -432.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.25 | 0.00 | 0.66 | 15.88 | 294.46 | 18.22 | 297.56 | 0.3408 | -860.0 | -711.8 | |
| 0.00 | 1.52 | 0.00 | 0.79 | 14.91 | 293.32 | 17.09 | 296.18 | 0.3177 | -702.0 | -425.5 | |
| 8.41 | 153.20 | 4.35 | 79.09 | 13.19 | 291.95 | 15.72 | 292.44 | 0.2867 | -1083.9 | -560.5 | |
| 8.05 | -3.00 | 4.17 | -3.00 | 14.04 | 291.85 | 15.62 | 295.35 | 0.2903 | -1067.6 | 999999 | |
| 11.18 | -3.00 | 5.78 | -3.00 | 13.56 | 291.72 | 15.49 | 293.95 | 0.2853 | -1148.5 | 999999 | |
| 6.71 | -3.00 | 3.46 | -3.00 | 13.23 | 291.63 | 15.40 | 292.95 | 0.2820 | -1265.2 | 999999 | |
| 2.33 | -3.00 | 1.20 | -3.00 | 13.33 | 291.35 | 15.12 | 293.64 | 0.2783 | -1286.5 | 999999 | |
| 0.00 | 4.47 | 0.00 | 2.29 | 11.59 | 290.67 | 14.44 | 288.23 | 0.2584 | 750.0 | 658.5 | |
| 0.00 | 1.07 | 0.00 | 0.55 | 13.64 | 287.92 | 11.68 | 300.25 | 0.2288 | 741.0 | 551.4 | |
| 0.00 | 2.33 | 0.00 | 1.19 | 15.05 | 287.61 | 11.38 | 306.13 | 0.2369 | 892.0 | 723.7 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 15.54 | 287.35 | 11.11 | 308.45 | 0.2382 | 872.0 | 727.0 | |
| 0.00 | 3.31 | 0.00 | 1.69 | 16.04 | 287.09 | 10.85 | 310.75 | 0.2400 | 1046.0 | 715.9 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 16.60 | 286.73 | 10.50 | 313.45 | 0.2416 | 862.0 | 618.5 | |
| 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. | |