| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.52 | 70.44 | 20.67 | 37.77 | 18.00 | 214.53 | -15.38 | 41.47 | 0.3823 | 421.9 | 407.7 | |
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back to the solar disc SDO HMI 2011-11-26 03:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.82 | 218.29 | -11.62 | 34.34 | 0.3416 | 937.0 | 772.3 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.48 | 218.15 | -11.76 | 35.24 | 0.3384 | 883.0 | 730.7 | |
| 0.00 | 3.85 | 0.00 | 2.03 | 17.51 | 217.83 | -12.08 | 35.90 | 0.3418 | 772.0 | 653.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.27 | 217.66 | -12.25 | 36.74 | 0.3403 | 675.0 | 577.4 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 19.21 | 217.07 | -12.84 | 34.62 | 0.3711 | 750.0 | 590.7 | |
| 9.93 | 12.59 | 5.25 | 6.66 | 17.07 | 216.31 | -13.61 | 39.95 | 0.3517 | -992.6 | -674.5 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 19.86 | 215.85 | -14.06 | 35.96 | 0.3908 | 740.0 | 576.7 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 21.74 | 215.64 | -14.27 | 33.51 | 0.4166 | 849.0 | 677.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.13 | 215.82 | -14.09 | 40.80 | 0.3575 | -745.0 | -586.3 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 19.29 | 215.61 | -14.30 | 37.34 | 0.3861 | 904.0 | 694.6 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 17.50 | 215.70 | -14.21 | 40.35 | 0.3633 | -836.0 | -642.7 | |
| 0.00 | 2.14 | 0.00 | 1.16 | 21.48 | 215.30 | -14.61 | 34.48 | 0.4164 | 792.0 | 570.6 | |
| 2.91 | 3.42 | 1.55 | 1.83 | 18.15 | 215.26 | -14.65 | 40.00 | 0.3756 | -901.9 | -706.0 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 18.08 | 214.94 | -14.97 | 40.70 | 0.3782 | -698.0 | -518.0 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 17.83 | 213.96 | -15.95 | 42.91 | 0.3858 | 808.0 | 645.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 16.90 | 213.56 | -16.35 | 45.37 | 0.3801 | 709.0 | 513.1 | |
| 25.68 | 34.16 | 13.87 | 18.44 | 17.94 | 212.79 | -17.12 | 44.67 | 0.4002 | 1059.5 | 851.1 | |
| 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. | |