| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.37 | 188.71 | 20.93 | 111.63 | 18.46 | 103.06 | 28.00 | 305.35 | 0.5480 | -393.9 | -272.5 | |
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back to the solar disc SDO HMI 2011-12-07 21:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.11 | 7.76 | 0.66 | 4.59 | 17.07 | 104.15 | 29.08 | 302.20 | 0.5513 | 759.7 | 670.3 | |
| 2.39 | -1.00 | 1.41 | -1.00 | 16.89 | 103.98 | 28.91 | 302.04 | 0.5479 | 784.1 | 999999 | |
| 5.11 | 7.93 | 3.01 | 4.67 | 16.98 | 103.60 | 28.54 | 302.49 | 0.5439 | 766.7 | 446.9 | |
| 22.07 | 135.43 | 13.12 | 80.57 | 18.78 | 103.46 | 28.40 | 305.48 | 0.5551 | -1212.9 | -364.7 | |
| 0.00 | 2.39 | 0.00 | 1.40 | 16.76 | 103.04 | 27.98 | 302.61 | 0.5354 | 701.0 | 594.6 | |
| 1.28 | 4.43 | 0.75 | 2.58 | 17.69 | 102.04 | 26.98 | 305.02 | 0.5298 | -845.8 | -286.6 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 15.60 | 101.72 | 26.66 | 301.79 | 0.5105 | 541.0 | 402.1 | |
| 1.53 | -6.00 | 0.89 | -6.00 | 17.66 | 101.79 | 26.73 | 305.20 | 0.5266 | 509.4 | 999999 | |
| 0.00 | 3.41 | 0.00 | 2.00 | 19.00 | 101.60 | 26.53 | 307.53 | 0.5348 | -763.0 | -706.0 | |
| 1.88 | 21.65 | 1.09 | 12.57 | 18.31 | 101.27 | 26.21 | 306.76 | 0.5254 | -1115.4 | -299.9 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 14.65 | 99.53 | 24.46 | 302.15 | 0.4752 | 664.0 | 543.9 | |
| 0.00 | 3.15 | 0.00 | 1.79 | 16.27 | 99.43 | 24.37 | 305.17 | 0.4865 | 922.0 | 561.5 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 20.03 | 99.45 | 24.38 | 311.37 | 0.5189 | 724.0 | 548.2 | |
| 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. | |