| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.00 | 238.08 | 19.96 | 118.85 | 13.93 | 291.40 | 1.96 | 343.75 | 0.1245 | -597.8 | -366.3 | |
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back to the solar disc SDO HMI 2011-08-31 18:59:08 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.59 | 0.00 | 1.31 | 18.59 | 293.59 | 4.15 | 340.92 | 0.2107 | 770.0 | 699.3 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 18.01 | 293.35 | 3.91 | 340.98 | 0.2000 | 998.0 | 764.9 | |
| 5.55 | 216.71 | 2.77 | 108.12 | 14.22 | 291.90 | 2.46 | 341.25 | 0.1302 | -1167.0 | -500.4 | |
| 10.47 | -3.00 | 5.22 | -3.00 | 13.34 | 291.86 | 2.42 | 339.05 | 0.1156 | -1295.8 | 999999 | |
| 18.07 | -3.00 | 9.02 | -3.00 | 13.67 | 291.62 | 2.18 | 341.95 | 0.1196 | -1372.8 | 999999 | |
| 5.91 | -3.00 | 2.95 | -3.00 | 14.04 | 291.53 | 2.09 | 343.54 | 0.1252 | -1179.0 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 11.25 | 289.25 | -0.19 | 2.59 | 0.0714 | 953.0 | 769.9 | |
| 0.00 | 3.76 | 0.00 | 1.88 | 15.20 | 287.62 | -1.82 | 12.38 | 0.1436 | 1146.0 | 779.7 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 15.11 | 287.40 | -2.04 | 13.97 | 0.1429 | 903.0 | 752.9 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 14.74 | 287.41 | -2.04 | 14.62 | 0.1367 | 905.0 | 761.4 | |
| 0.00 | 2.15 | 0.00 | 1.08 | 15.81 | 286.86 | -2.58 | 16.09 | 0.1570 | 1012.0 | 782.2 | |
| 0.00 | 6.35 | 0.00 | 3.19 | 16.48 | 286.63 | -2.81 | 16.20 | 0.1693 | 936.0 | 688.9 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 16.42 | 286.22 | -3.22 | 18.53 | 0.1703 | 921.0 | 717.8 | |
| 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. | |