| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.35 | 155.09 | 41.58 | 88.05 | -25.18 | 85.32 | 5.58 | 190.32 | 0.4899 | -71.8 | -122.7 | |
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back to the solar disc SDO HMI 2011-11-10 05:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.59 | -25.64 | 89.14 | 9.41 | 196.89 | 0.5092 | -559.0 | -408.1 | |
| 25.08 | 60.43 | 14.38 | 34.67 | -25.73 | 87.88 | 8.14 | 194.69 | 0.5054 | 1137.9 | 251.5 | |
| 0.00 | 1.64 | 0.00 | 0.93 | -25.22 | 87.44 | 7.71 | 194.22 | 0.4962 | 737.0 | 832.5 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -24.85 | 87.29 | 7.56 | 194.15 | 0.4902 | 962.0 | 761.8 | |
| 5.26 | 6.21 | 2.96 | 3.49 | -24.03 | 86.36 | 6.62 | 192.87 | 0.4747 | 955.3 | 734.4 | |
| 0.00 | 1.47 | 0.00 | 0.84 | -26.37 | 86.49 | 6.75 | 191.97 | 0.5098 | 755.0 | 509.0 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -25.00 | 85.62 | 5.88 | 191.04 | 0.4869 | 633.0 | 497.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -23.99 | 85.05 | 5.31 | 190.41 | 0.4700 | 563.0 | 484.9 | |
| 0.00 | 2.50 | 0.00 | 1.40 | -23.89 | 84.68 | 4.95 | 189.76 | 0.4675 | 158.0 | 36.9 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -23.82 | 84.26 | 4.52 | 188.96 | 0.4654 | -475.0 | -413.1 | |
| 13.36 | 24.48 | 7.47 | 13.70 | -23.95 | 83.77 | 4.04 | 187.97 | 0.4663 | -1096.7 | -644.7 | |
| 0.00 | 1.47 | 0.00 | 0.82 | -24.52 | 83.76 | 4.03 | 187.76 | 0.4750 | -149.0 | -216.4 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -26.04 | 83.48 | 3.75 | 186.80 | 0.4975 | -492.0 | -400.9 | |
| 1.03 | 43.88 | 0.59 | 24.86 | -25.57 | 83.30 | 3.57 | 186.60 | 0.4900 | -736.8 | -672.5 | |
| 15.00 | -14.00 | 8.49 | -14.00 | -25.36 | 82.96 | 3.23 | 186.03 | 0.4863 | -1049.6 | 999999 | |
| 5.17 | 7.24 | 2.91 | 4.08 | -24.85 | 82.75 | 3.02 | 185.76 | 0.4782 | -1055.2 | -795.6 | |
| 8.45 | -14.00 | 4.78 | -14.00 | -25.43 | 82.44 | 2.71 | 185.05 | 0.4866 | -924.3 | 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. | |