| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.35 | 171.53 | 25.17 | 112.38 | 18.74 | 103.21 | 36.91 | 299.49 | 0.6561 | -361.9 | -218.7 | |
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back to the solar disc SDO HMI 2011-12-08 13:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.80 | 17.77 | 105.36 | 39.05 | 296.98 | 0.6757 | 594.0 | 472.6 | |
| 11.42 | 19.43 | 7.59 | 12.91 | 17.40 | 104.98 | 38.68 | 296.65 | 0.6696 | 867.3 | 727.7 | |
| 0.00 | 0.85 | 0.00 | 0.56 | 16.93 | 103.77 | 37.46 | 296.61 | 0.6532 | 418.0 | 446.3 | |
| 21.99 | 120.07 | 14.42 | 78.81 | 18.76 | 103.36 | 37.06 | 299.44 | 0.6575 | -1086.8 | -293.0 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 17.21 | 102.79 | 36.48 | 297.54 | 0.6429 | -633.0 | -581.2 | |
| 0.00 | 0.85 | 0.00 | 0.57 | 21.82 | 102.95 | 36.65 | 303.88 | 0.6698 | -789.0 | -616.4 | |
| 4.94 | 16.36 | 3.16 | 10.44 | 17.86 | 101.82 | 35.52 | 299.04 | 0.6348 | -774.0 | -322.0 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 18.17 | 101.67 | 35.36 | 299.58 | 0.6346 | -737.0 | -610.0 | |
| 0.00 | 1.53 | 0.00 | 0.98 | 18.23 | 101.34 | 35.03 | 299.87 | 0.6311 | -857.0 | -673.8 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 19.26 | 101.01 | 34.71 | 301.56 | 0.6332 | -572.0 | -558.2 | |
| 0.00 | 1.45 | 0.00 | 0.90 | 16.86 | 99.58 | 33.28 | 298.95 | 0.6024 | 575.0 | 428.0 | |
| 0.00 | 1.45 | 0.00 | 0.99 | 26.52 | 102.21 | 35.91 | 310.41 | 0.6916 | -449.0 | -397.0 | |
| 0.00 | 1.19 | 0.00 | 0.74 | 16.71 | 99.40 | 33.10 | 298.83 | 0.5993 | 814.0 | 651.8 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 18.94 | 98.10 | 31.79 | 303.11 | 0.5972 | 657.0 | 542.2 | |
| 0.00 | 2.56 | 0.00 | 1.73 | 28.18 | 100.01 | 33.71 | 314.01 | 0.6825 | -729.0 | -498.9 | |
| 0.00 | 0.85 | 0.00 | 0.58 | 28.68 | 99.59 | 33.28 | 314.93 | 0.6824 | -571.0 | -469.4 | |
| 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. | |