| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.67 | 306.01 | 22.79 | 167.41 | 28.05 | 43.17 | 2.44 | 354.92 | 0.4256 | -925.0 | -434.8 | |
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back to the solar disc SDO HMI 2011-11-13 04:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.21 | 294.21 | 0.66 | 160.96 | 27.88 | 44.06 | 3.33 | 353.01 | 0.4241 | -810.3 | -446.6 | |
| 9.64 | -1.00 | 5.28 | -1.00 | 28.21 | 43.53 | 2.80 | 354.20 | 0.4284 | -1182.6 | 999999 | |
| 21.78 | -1.00 | 11.89 | -1.00 | 27.88 | 43.39 | 2.66 | 354.41 | 0.4230 | -1451.0 | 999999 | |
| 3.36 | -1.00 | 1.84 | -1.00 | 28.18 | 43.13 | 2.40 | 355.03 | 0.4273 | -1020.9 | 999999 | |
| 4.99 | -1.00 | 2.74 | -1.00 | 28.44 | 43.00 | 2.27 | 355.35 | 0.4312 | -854.6 | 999999 | |
| 0.69 | -1.00 | 0.38 | -1.00 | 28.18 | 42.69 | 1.96 | 355.93 | 0.4267 | -866.0 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 28.12 | 40.97 | 0.24 | 359.49 | 0.4246 | -766.0 | -591.8 | |
| 0.00 | 1.81 | 0.00 | 1.00 | 29.17 | 40.46 | -0.26 | 0.52 | 0.4413 | -628.0 | -539.8 | |
| 0.00 | 3.53 | 0.00 | 1.94 | 28.91 | 40.43 | -0.30 | 0.60 | 0.4371 | -853.0 | -685.6 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 29.10 | 40.29 | -0.43 | 0.86 | 0.4403 | -753.0 | -630.6 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 27.92 | 37.58 | -3.15 | 6.60 | 0.4243 | 775.0 | 600.2 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 27.69 | 37.48 | -3.24 | 6.87 | 0.4209 | 713.0 | 578.9 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 25.67 | 36.12 | -4.61 | 10.67 | 0.3924 | 686.0 | 662.0 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 23.20 | 33.03 | -7.70 | 19.69 | 0.3670 | 865.0 | 592.3 | |
| 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. | |