| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.54 | 49.04 | 11.70 | 54.30 | -17.15 | 340.20 | 61.39 | 249.66 | 0.8962 | 295.4 | 151.2 | |
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back to the solar disc SDO HMI 2011-11-22 10:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 7.03 | 0.00 | 8.17 | -16.46 | 341.76 | 62.95 | 250.75 | 0.9065 | -474.0 | -338.9 | |
| 0.00 | 1.71 | 0.00 | 1.97 | -16.97 | 341.38 | 62.57 | 250.11 | 0.9046 | 270.0 | 246.4 | |
| 0.00 | 0.94 | 0.00 | 1.11 | -17.95 | 341.71 | 62.90 | 249.11 | 0.9082 | -125.0 | -153.0 | |
| 0.00 | 1.46 | 0.00 | 1.66 | -17.52 | 340.90 | 62.09 | 249.42 | 0.9020 | 577.0 | 411.6 | |
| 10.54 | 25.89 | 11.70 | 28.60 | -16.63 | 340.32 | 61.51 | 250.28 | 0.8965 | 621.8 | 448.3 | |
| 0.00 | 0.86 | 0.00 | 0.99 | -18.06 | 341.17 | 62.35 | 248.88 | 0.9046 | -119.0 | -92.8 | |
| 0.00 | 2.66 | 0.00 | 3.02 | -17.71 | 340.81 | 62.00 | 249.20 | 0.9016 | 242.0 | 234.5 | |
| 0.00 | 1.11 | 0.00 | 1.25 | -18.29 | 340.30 | 61.49 | 248.46 | 0.8989 | -288.0 | -197.5 | |
| 0.00 | 0.60 | 0.00 | 0.66 | -18.58 | 339.57 | 60.76 | 247.98 | 0.8941 | 313.0 | 196.9 | |
| 0.00 | 3.17 | 0.00 | 3.43 | -18.63 | 339.15 | 60.34 | 247.83 | 0.8911 | 550.0 | 416.2 | |
| 0.00 | 0.69 | 0.00 | 0.71 | -19.55 | 337.39 | 58.58 | 246.39 | 0.8797 | -360.0 | -354.1 | |
| 0.00 | 1.89 | 0.00 | 1.92 | -19.35 | 336.91 | 58.10 | 246.49 | 0.8756 | -471.0 | -413.5 | |
| 0.00 | 1.03 | 0.00 | 0.81 | -21.09 | 325.60 | 46.78 | 240.68 | 0.7822 | -388.0 | -312.8 | |
| 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. | |