| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.68 | 57.59 | 22.65 | 175.26 | -23.46 | 284.50 | -78.32 | 114.39 | 0.9856 | 244.9 | 20.5 | |
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back to the solar disc SDO HMI 2011-11-16 01:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.19 | 52.52 | 15.96 | 139.92 | -23.37 | 286.13 | -76.69 | 114.46 | 0.9823 | 498.7 | 59.1 | |
| 2.49 | -1.00 | 6.69 | -1.00 | -23.32 | 285.62 | -77.20 | 114.36 | 0.9838 | -214.2 | 999999 | |
| 0.00 | 1.80 | 0.00 | 5.14 | -22.78 | 284.87 | -77.95 | 113.71 | 0.9856 | -308.0 | -221.0 | |
| 0.00 | 3.27 | 0.00 | 30.20 | -24.05 | 277.59 | -85.23 | 114.30 | 0.9987 | -181.0 | -88.4 | |
| 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. | |