| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.84 | 47.32 | 23.02 | 57.33 | 16.82 | 297.27 | 65.16 | 287.78 | 0.9130 | 12.5 | 103.4 | |
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back to the solar disc SDO HMI 2011-11-25 23:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.19 | 13.10 | 9.99 | 18.29 | 16.44 | 300.82 | 68.72 | 287.00 | 0.9361 | -404.0 | 13.9 | |
| 0.00 | 2.14 | 0.00 | 2.91 | 15.86 | 300.31 | 68.21 | 286.43 | 0.9328 | -481.0 | -303.4 | |
| 0.00 | 1.54 | 0.00 | 1.90 | 15.92 | 297.96 | 65.85 | 286.71 | 0.9179 | -333.0 | -241.3 | |
| 0.00 | 1.28 | 0.00 | 1.56 | 16.37 | 297.42 | 65.31 | 287.25 | 0.9145 | -433.0 | -378.5 | |
| 1.46 | 2.65 | 1.63 | 2.98 | 16.17 | 295.29 | 63.18 | 287.27 | 0.8995 | 148.9 | 15.5 | |
| 1.03 | 2.57 | 1.16 | 2.90 | 16.66 | 295.44 | 63.33 | 287.79 | 0.9010 | 213.2 | 144.7 | |
| 1.28 | 2.14 | 1.44 | 2.39 | 16.39 | 295.14 | 63.03 | 287.53 | 0.8986 | 335.0 | 214.6 | |
| 4.37 | 5.05 | 4.92 | 5.70 | 17.37 | 295.25 | 63.15 | 288.60 | 0.9003 | 374.6 | 162.0 | |
| 0.00 | 2.82 | 0.00 | 3.14 | 16.83 | 294.85 | 62.74 | 288.05 | 0.8968 | 433.0 | 336.2 | |
| 0.00 | 2.05 | 0.00 | 2.28 | 17.14 | 294.76 | 62.66 | 288.41 | 0.8965 | 276.0 | 314.2 | |
| 3.51 | 5.22 | 3.88 | 5.78 | 17.51 | 294.65 | 62.54 | 288.84 | 0.8960 | 565.3 | 574.0 | |
| 0.00 | 5.39 | 0.00 | 6.01 | 17.88 | 294.88 | 62.77 | 289.21 | 0.8980 | 659.0 | 389.6 | |
| 0.00 | 0.51 | 0.00 | 0.56 | 16.84 | 294.25 | 62.14 | 288.14 | 0.8924 | -455.0 | -443.8 | |
| 0.00 | 0.86 | 0.00 | 0.93 | 17.96 | 293.98 | 61.88 | 289.43 | 0.8915 | -251.0 | -207.6 | |
| 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. | |