| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.32 | 184.79 | 27.32 | 112.09 | -25.33 | 86.94 | 20.94 | 213.97 | 0.5781 | 10.4 | 136.9 | |
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back to the solar disc SDO HMI 2011-11-11 06:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.11 | 130.95 | 9.91 | 80.50 | -25.48 | 88.95 | 22.95 | 216.39 | 0.5955 | 1043.8 | 365.2 | |
| 7.93 | -1.00 | 4.86 | -1.00 | -25.63 | 88.38 | 22.37 | 215.56 | 0.5924 | 971.9 | 999999 | |
| 1.38 | -1.00 | 0.84 | -1.00 | -25.69 | 87.96 | 21.96 | 215.00 | 0.5896 | 730.4 | 999999 | |
| 1.55 | -1.00 | 0.94 | -1.00 | -25.21 | 87.76 | 21.76 | 215.29 | 0.5828 | 914.7 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.05 | -25.99 | 87.56 | 21.55 | 214.20 | 0.5897 | 821.0 | 619.2 | |
| 0.00 | 2.84 | 0.00 | 1.69 | -24.69 | 85.43 | 19.43 | 212.93 | 0.5581 | -1024.0 | -675.1 | |
| 0.00 | 1.98 | 0.00 | 1.17 | -24.00 | 84.63 | 18.63 | 212.61 | 0.5437 | 701.0 | 669.3 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -23.86 | 83.93 | 17.92 | 211.79 | 0.5364 | -817.0 | -678.0 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -23.84 | 83.21 | 17.21 | 210.79 | 0.5307 | -622.0 | -566.7 | |
| 0.00 | 4.31 | 0.00 | 2.51 | -23.80 | 82.86 | 16.86 | 210.33 | 0.5276 | -1118.0 | -886.0 | |
| 0.00 | 2.15 | 0.00 | 1.27 | -25.48 | 82.79 | 16.79 | 208.53 | 0.5480 | -703.0 | -660.8 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -25.85 | 82.67 | 16.67 | 208.01 | 0.5518 | -532.0 | -414.7 | |
| 13.87 | 19.90 | 8.15 | 11.69 | -25.30 | 81.98 | 15.97 | 207.55 | 0.5401 | -938.5 | -657.2 | |
| 4.48 | 12.49 | 2.62 | 7.29 | -24.66 | 81.89 | 15.89 | 208.04 | 0.5313 | -1032.7 | -765.8 | |
| 0.00 | 1.38 | 0.00 | 0.80 | -24.72 | 81.56 | 15.56 | 207.49 | 0.5298 | -952.0 | -731.0 | |
| 0.00 | 2.76 | 0.00 | 1.60 | -24.18 | 81.19 | 15.18 | 207.46 | 0.5203 | -808.0 | -653.7 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -24.47 | 80.99 | 14.98 | 206.87 | 0.5228 | -736.0 | -610.7 | |
| 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. | |