| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.18 | 225.51 | 25.04 | 134.09 | 9.21 | 357.16 | -32.35 | 72.53 | 0.5558 | -643.2 | -295.3 | |
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back to the solar disc SDO HMI 2011-12-11 08:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.59 | 7.84 | 358.88 | -30.63 | 74.25 | 0.5265 | 638.0 | 348.8 | |
| 31.52 | 182.92 | 18.63 | 108.11 | 9.40 | 357.80 | -31.72 | 71.93 | 0.5477 | -1177.5 | -443.9 | |
| 5.03 | -2.00 | 2.99 | -2.00 | 9.02 | 357.23 | -32.28 | 72.88 | 0.5540 | -761.1 | 999999 | |
| 0.00 | 2.04 | 0.00 | 1.22 | 9.53 | 356.79 | -32.72 | 72.19 | 0.5621 | -484.0 | -329.6 | |
| 1.11 | 5.45 | 0.66 | 3.25 | 8.90 | 356.78 | -32.73 | 73.28 | 0.5599 | -660.0 | -585.1 | |
| 0.00 | 1.19 | 0.00 | 0.71 | 7.97 | 356.59 | -32.92 | 74.98 | 0.5595 | -575.0 | -444.1 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 8.78 | 356.33 | -33.18 | 73.68 | 0.5657 | -635.0 | -506.2 | |
| 0.00 | 1.62 | 0.00 | 0.98 | 8.55 | 355.39 | -34.12 | 74.46 | 0.5780 | -594.0 | -559.9 | |
| 0.00 | 2.39 | 0.00 | 1.45 | 9.92 | 355.20 | -34.31 | 72.23 | 0.5854 | 826.0 | 509.2 | |
| 2.22 | 3.92 | 1.34 | 2.38 | 8.82 | 355.29 | -34.22 | 74.05 | 0.5803 | -738.1 | -724.5 | |
| 0.00 | 14.82 | 0.00 | 9.09 | 8.37 | 354.35 | -35.16 | 75.14 | 0.5917 | 862.0 | 700.4 | |
| 1.11 | 3.92 | 0.68 | 2.42 | 8.61 | 353.77 | -35.74 | 74.95 | 0.6003 | 935.1 | 768.8 | |
| 0.00 | 1.53 | 0.00 | 0.95 | 8.08 | 353.68 | -35.83 | 75.86 | 0.5999 | 658.0 | 576.1 | |
| 1.19 | 1.79 | 0.74 | 1.11 | 8.67 | 353.47 | -36.04 | 74.95 | 0.6045 | 646.8 | 617.9 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 8.48 | 350.36 | -39.15 | 76.26 | 0.6452 | 722.0 | 533.2 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 8.21 | 350.16 | -39.35 | 76.72 | 0.6472 | 566.0 | 457.4 | |
| 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. | |