| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.36 | 79.62 | 17.46 | 41.61 | 17.83 | 214.47 | -8.88 | 27.26 | 0.3202 | 487.1 | 383.5 | |
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back to the solar disc SDO HMI 2011-11-26 15:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.88 | 218.44 | -4.90 | 16.08 | 0.2950 | 829.0 | 608.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.97 | 218.10 | -5.25 | 17.05 | 0.2981 | 804.0 | 690.2 | |
| 0.00 | 2.14 | 0.00 | 1.11 | 17.54 | 217.95 | -5.39 | 17.95 | 0.2920 | 894.0 | 871.7 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 17.85 | 217.85 | -5.49 | 17.93 | 0.2974 | 807.0 | 735.6 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 17.63 | 217.76 | -5.58 | 18.43 | 0.2944 | 944.0 | 762.3 | |
| 7.27 | 18.13 | 3.76 | 9.37 | 16.74 | 216.83 | -6.52 | 22.44 | 0.2860 | -1046.6 | -495.2 | |
| 1.54 | -6.00 | 0.80 | -6.00 | 16.83 | 216.55 | -6.80 | 23.18 | 0.2892 | -705.5 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 21.11 | 215.95 | -7.39 | 19.67 | 0.3583 | 819.0 | 654.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.17 | 215.73 | -7.62 | 20.15 | 0.3605 | 891.0 | 659.3 | |
| 0.00 | 2.05 | 0.00 | 1.06 | 16.55 | 215.72 | -7.63 | 26.08 | 0.2908 | -1047.0 | -804.2 | |
| 0.00 | 2.40 | 0.00 | 1.25 | 18.27 | 215.61 | -7.73 | 23.86 | 0.3173 | -1015.0 | -751.9 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 22.08 | 214.77 | -8.57 | 21.43 | 0.3797 | 650.0 | 504.6 | |
| 2.91 | 46.70 | 1.53 | 24.52 | 18.08 | 213.23 | -10.12 | 30.30 | 0.3325 | 997.6 | 825.9 | |
| 21.64 | -13.00 | 11.37 | -13.00 | 18.04 | 212.82 | -10.53 | 31.34 | 0.3355 | 1035.5 | 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. | |