| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.59 | 27.66 | 5.62 | 16.35 | -27.39 | 234.85 | -23.27 | 140.05 | 0.5479 | 292.4 | 129.3 | |
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back to the solar disc SDO HMI 2010-12-31 18:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.30 | 12.57 | 4.28 | 7.36 | -27.85 | 236.58 | -21.53 | 142.59 | 0.5364 | 866.9 | 745.9 | |
| 2.29 | -1.00 | 1.34 | -1.00 | -27.59 | 236.53 | -21.59 | 142.19 | 0.5340 | 885.0 | 999999 | |
| 0.00 | 0.93 | 0.00 | 0.54 | -26.74 | 236.17 | -21.95 | 140.64 | 0.5284 | 628.0 | 531.7 | |
| 0.00 | 1.95 | 0.00 | 1.15 | -27.46 | 234.90 | -23.21 | 140.13 | 0.5477 | -699.0 | -495.2 | |
| 0.00 | 2.12 | 0.00 | 1.24 | -25.88 | 234.88 | -23.23 | 137.95 | 0.5320 | 749.0 | 546.2 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -25.77 | 234.26 | -23.85 | 137.11 | 0.5371 | 707.0 | 626.7 | |
| 0.00 | 0.93 | 0.00 | 0.56 | -27.86 | 233.79 | -24.32 | 139.44 | 0.5622 | -622.0 | -476.4 | |
| 0.00 | 0.93 | 0.00 | 0.55 | -25.60 | 233.97 | -24.14 | 136.56 | 0.5384 | 635.0 | 484.5 | |
| 0.00 | 1.87 | 0.00 | 1.11 | -27.17 | 233.29 | -24.82 | 137.99 | 0.5602 | 916.0 | 647.1 | |
| 0.00 | 1.78 | 0.00 | 1.08 | -28.22 | 232.00 | -26.11 | 138.06 | 0.5825 | -619.0 | -529.1 | |
| 0.00 | 0.76 | 0.00 | 0.46 | -27.65 | 231.55 | -26.56 | 136.87 | 0.5816 | -631.0 | -581.8 | |
| 0.00 | 1.44 | 0.00 | 0.88 | -27.64 | 231.14 | -26.97 | 136.47 | 0.5855 | -413.0 | -371.4 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -27.77 | 231.00 | -27.12 | 136.50 | 0.5881 | -687.0 | -564.8 | |
| 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. | |