| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.46 | 80.66 | 15.90 | 42.09 | 18.09 | 214.69 | -7.55 | 23.45 | 0.3152 | 564.4 | 362.8 | |
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back to the solar disc SDO HMI 2011-11-26 17:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.48 | 0.00 | 1.33 | 23.81 | 218.60 | -3.64 | 8.70 | 0.3859 | 805.0 | 641.2 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 17.54 | 218.44 | -3.81 | 12.89 | 0.2850 | 691.0 | 668.8 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.20 | 218.35 | -3.89 | 13.46 | 0.2798 | 961.0 | 745.2 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 17.01 | 218.17 | -4.07 | 14.23 | 0.2775 | 931.0 | 690.8 | |
| 0.00 | 4.62 | 0.00 | 2.39 | 17.87 | 218.02 | -4.22 | 13.93 | 0.2921 | 872.0 | 689.1 | |
| 4.88 | 12.74 | 2.51 | 6.57 | 16.67 | 216.94 | -5.30 | 18.67 | 0.2779 | -1089.5 | -576.7 | |
| 0.00 | 3.34 | 0.00 | 1.72 | 16.70 | 216.59 | -5.65 | 19.74 | 0.2803 | -983.0 | -797.4 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.17 | 216.23 | -6.01 | 18.03 | 0.3210 | 1021.0 | 747.0 | |
| 0.00 | 1.80 | 0.00 | 0.95 | 21.04 | 215.90 | -6.34 | 17.10 | 0.3519 | 729.0 | 619.2 | |
| 0.00 | 3.59 | 0.00 | 1.90 | 21.14 | 215.61 | -6.63 | 17.75 | 0.3548 | 675.0 | 674.5 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.27 | 215.67 | -6.57 | 20.62 | 0.3101 | -941.0 | -753.9 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 16.55 | 215.70 | -6.54 | 22.78 | 0.2833 | -1028.0 | -851.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.25 | 213.49 | -8.75 | 28.13 | 0.3097 | 781.0 | 581.2 | |
| 2.91 | 43.79 | 1.52 | 22.92 | 18.08 | 213.20 | -9.05 | 27.61 | 0.3240 | 978.5 | 846.4 | |
| 22.67 | -14.00 | 11.87 | -14.00 | 18.01 | 212.82 | -9.42 | 28.66 | 0.3260 | 1051.3 | 999999 | |
| 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. | |