SDO HMI 2011-12-05 18:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.95 | 0.00 | 10.97 | 20.26 | 86.94 | -16.14 | 36.93 | 0.4321 | -16.0 | -108.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.39 | 0.00 | 1.26 | 16.51 | 91.50 | -11.58 | 34.64 | 0.3401 | -719.0 | -598.6 | |
| 0.00 | 1.96 | 0.00 | 1.08 | 22.77 | 90.17 | -12.90 | 28.35 | 0.4355 | -799.0 | -527.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 19.42 | 90.40 | -12.67 | 32.32 | 0.3887 | -873.0 | -555.6 | |
| 0.00 | 2.81 | 0.00 | 1.53 | 20.36 | 89.16 | -13.92 | 33.36 | 0.4118 | -841.0 | -754.1 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 19.83 | 89.11 | -13.97 | 34.23 | 0.4054 | -872.0 | -693.3 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 19.67 | 89.09 | -13.98 | 34.49 | 0.4035 | -854.0 | -702.7 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 20.14 | 88.99 | -14.09 | 34.00 | 0.4105 | -679.0 | -618.0 | |
| 0.00 | 1.62 | 0.00 | 0.90 | 19.92 | 84.46 | -18.62 | 41.84 | 0.4520 | 731.0 | 525.3 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 20.83 | 83.54 | -19.54 | 41.75 | 0.4715 | 703.0 | 592.3 | |
| 0.00 | 1.79 | 0.00 | 1.00 | 20.45 | 83.45 | -19.62 | 42.44 | 0.4682 | 892.0 | 724.4 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 20.54 | 82.43 | -20.65 | 43.69 | 0.4800 | 924.0 | 772.3 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 20.45 | 82.18 | -20.90 | 44.17 | 0.4817 | 803.0 | 627.6 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 21.68 | 81.21 | -21.87 | 43.54 | 0.5045 | 673.0 | 555.2 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 24.30 | 80.12 | -22.96 | 41.17 | 0.5422 | 687.0 | 602.8 | |
| 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. | |