| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.77 | 170.11 | 22.67 | 110.57 | 18.46 | 103.29 | 36.44 | 299.37 | 0.6487 | -320.6 | -215.5 | |
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back to the solar disc SDO HMI 2011-12-08 12:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.62 | 17.71 | 105.29 | 38.44 | 297.21 | 0.6683 | 585.0 | 503.6 | |
| 11.25 | 20.45 | 7.42 | 13.47 | 17.36 | 104.93 | 38.08 | 296.91 | 0.6625 | 895.2 | 717.9 | |
| 0.00 | 0.94 | 0.00 | 0.61 | 16.93 | 103.74 | 36.88 | 296.92 | 0.6463 | 491.0 | 453.2 | |
| 20.11 | 123.15 | 13.09 | 80.29 | 18.73 | 103.36 | 36.50 | 299.71 | 0.6509 | -1127.1 | -290.0 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 17.05 | 102.96 | 36.10 | 297.53 | 0.6375 | -415.0 | -367.7 | |
| 0.00 | 1.53 | 0.00 | 0.98 | 17.21 | 102.84 | 35.98 | 297.82 | 0.6369 | -545.0 | -549.7 | |
| 0.00 | 1.19 | 0.00 | 0.79 | 21.85 | 102.95 | 36.10 | 304.26 | 0.6640 | -633.0 | -535.4 | |
| 3.41 | 12.44 | 2.16 | 7.89 | 17.86 | 101.76 | 34.91 | 299.40 | 0.6276 | -888.7 | -442.5 | |
| 0.00 | 1.28 | 0.00 | 0.81 | 18.20 | 101.65 | 34.80 | 299.97 | 0.6282 | -778.0 | -663.4 | |
| 0.00 | 2.81 | 0.00 | 1.78 | 18.29 | 101.30 | 34.44 | 300.33 | 0.6245 | -712.0 | -669.7 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 19.23 | 101.06 | 34.21 | 301.84 | 0.6272 | -757.0 | -657.8 | |
| 0.00 | 1.96 | 0.00 | 1.20 | 16.65 | 99.39 | 32.54 | 299.10 | 0.5920 | 896.0 | 720.7 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 18.97 | 98.58 | 31.72 | 303.21 | 0.5966 | 657.0 | 489.6 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 18.94 | 98.06 | 31.20 | 303.55 | 0.5902 | 447.0 | 476.7 | |
| 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. | |