| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.70 | 84.61 | 17.77 | 43.29 | 7.86 | 42.84 | -11.93 | 55.47 | 0.2491 | 298.4 | -96.9 | |
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back to the solar disc SDO HMI 2011-12-09 10:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.05 | 10.82 | 1.04 | 5.49 | 7.71 | 45.13 | -9.65 | 50.54 | 0.2161 | -1117.3 | -1012.3 | |
| 3.92 | 20.45 | 1.99 | 10.39 | 7.23 | 44.62 | -10.15 | 53.69 | 0.2179 | -1012.5 | -871.5 | |
| 4.52 | -2.00 | 2.29 | -2.00 | 7.71 | 44.55 | -10.22 | 52.14 | 0.2238 | -938.3 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 8.10 | 44.39 | -10.38 | 51.21 | 0.2300 | -825.0 | -675.1 | |
| 0.51 | 2.30 | 0.26 | 1.17 | 8.13 | 44.24 | -10.54 | 51.51 | 0.2323 | -878.2 | -628.7 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 8.13 | 43.87 | -10.90 | 52.45 | 0.2372 | -934.0 | -733.0 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 7.18 | 43.75 | -11.03 | 56.12 | 0.2296 | -354.0 | -273.6 | |
| 3.92 | 4.43 | 2.01 | 2.27 | 8.40 | 42.56 | -12.22 | 54.64 | 0.2579 | 1063.1 | 900.8 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 8.52 | 42.18 | -12.59 | 55.05 | 0.2641 | 878.0 | 619.2 | |
| 0.00 | 2.47 | 0.00 | 1.27 | 8.13 | 42.17 | -12.60 | 56.33 | 0.2608 | 1239.0 | 944.6 | |
| 0.00 | 1.87 | 0.00 | 0.96 | 7.41 | 41.82 | -12.95 | 59.38 | 0.2594 | 902.0 | 613.1 | |
| 8.61 | 37.50 | 4.43 | 19.31 | 7.89 | 41.41 | -13.36 | 58.59 | 0.2694 | 1151.4 | 723.2 | |
| 9.12 | -12.00 | 4.70 | -12.00 | 8.13 | 41.10 | -13.68 | 58.42 | 0.2760 | 1027.9 | 999999 | |
| 2.05 | -12.00 | 1.05 | -12.00 | 8.10 | 40.76 | -14.01 | 59.11 | 0.2806 | 807.5 | 999999 | |
| 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. | |