| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.73 | 32.70 | 18.60 | 57.14 | -18.64 | 80.25 | 72.72 | 250.70 | 0.9597 | 287.6 | 311.5 | |
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back to the solar disc SDO HMI 2011-12-13 00:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.53 | 3.92 | 3.11 | 7.93 | -18.39 | 82.80 | 75.27 | 251.17 | 0.9708 | 231.9 | 263.4 | |
| 0.00 | 2.55 | 0.00 | 4.78 | -18.96 | 81.48 | 73.96 | 250.48 | 0.9655 | 275.0 | 252.0 | |
| 3.32 | 26.23 | 5.67 | 44.43 | -18.38 | 79.95 | 72.42 | 250.95 | 0.9584 | 480.6 | 329.4 | |
| 3.07 | -3.00 | 5.15 | -3.00 | -18.66 | 79.63 | 72.10 | 250.63 | 0.9570 | 569.0 | 999999 | |
| 2.81 | -3.00 | 4.67 | -3.00 | -18.98 | 79.35 | 71.82 | 250.28 | 0.9558 | -217.1 | 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. | |