| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.02 | 45.79 | 24.14 | 117.94 | 7.90 | 245.73 | 79.18 | 277.25 | 0.9814 | -221.3 | -85.8 | |
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back to the solar disc SDO HMI 2011-11-03 15:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.28 | 25.49 | 8.98 | 71.84 | 7.56 | 246.53 | 79.98 | 276.93 | 0.9842 | -381.3 | -104.9 | |
| 0.00 | 1.47 | 0.00 | 3.97 | 9.19 | 246.50 | 79.95 | 278.59 | 0.9839 | -163.0 | -96.6 | |
| 1.64 | 11.23 | 3.81 | 25.19 | 8.22 | 244.74 | 78.19 | 277.53 | 0.9781 | -398.9 | 65.7 | |
| 2.59 | -3.00 | 5.70 | -3.00 | 8.10 | 243.93 | 77.38 | 277.36 | 0.9752 | 296.1 | 999999 | |
| 2.51 | 7.60 | 5.65 | 16.94 | 8.70 | 244.34 | 77.79 | 278.00 | 0.9766 | -379.4 | -185.8 | |
| 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. | |