| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.11 | 268.57 | 23.50 | 134.01 | 9.61 | 56.72 | 1.72 | 340.08 | 0.1187 | -1038.4 | -417.3 | |
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back to the solar disc SDO HMI 2011-11-12 02:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.06 | 241.54 | 21.47 | 120.43 | 9.43 | 57.15 | 2.15 | 341.11 | 0.1146 | -1505.4 | -461.9 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 7.38 | 56.81 | 1.80 | 336.61 | 0.0791 | -997.0 | -818.3 | |
| 0.60 | -1.00 | 0.30 | -1.00 | 9.37 | 56.58 | 1.57 | 345.78 | 0.1108 | -868.7 | 999999 | |
| 0.00 | 3.27 | 0.00 | 1.63 | 9.88 | 56.19 | 1.18 | 350.02 | 0.1180 | -1016.0 | -818.3 | |
| 0.00 | 1.55 | 0.00 | 0.78 | 11.25 | 56.17 | 1.16 | 351.90 | 0.1416 | -799.0 | -636.7 | |
| 0.00 | 1.21 | 0.00 | 0.60 | 10.78 | 55.68 | 0.67 | 354.96 | 0.1324 | -779.0 | -539.9 | |
| 2.33 | 11.28 | 1.17 | 5.66 | 12.13 | 55.17 | 0.16 | 358.98 | 0.1553 | -749.5 | 302.2 | |
| 1.12 | -7.00 | 0.56 | -7.00 | 12.28 | 55.08 | 0.07 | 359.56 | 0.1579 | 667.0 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 10.29 | 51.37 | -3.64 | 26.93 | 0.1386 | -1057.0 | -766.3 | |
| 0.00 | 1.89 | 0.00 | 0.95 | 10.29 | 50.91 | -4.09 | 29.74 | 0.1423 | -962.0 | -796.0 | |
| 0.00 | 1.46 | 0.00 | 0.74 | 12.74 | 49.84 | -5.17 | 27.97 | 0.1882 | 1042.0 | 903.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 12.46 | 47.09 | -7.91 | 39.91 | 0.2105 | 924.0 | 616.8 | |
| 0.00 | 1.46 | 0.00 | 0.74 | 8.25 | 45.23 | -9.78 | 62.29 | 0.1907 | 908.0 | 698.2 | |
| 0.00 | 1.55 | 0.00 | 0.79 | 12.00 | 43.41 | -11.59 | 52.01 | 0.2506 | 863.0 | 671.5 | |
| 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. | |