| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.68 | 171.40 | 54.39 | 459.32 | -23.02 | 107.27 | 78.85 | 246.64 | 0.9843 | 316.9 | 257.0 | |
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back to the solar disc SDO HMI 2011-12-11 10:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.60 | 0.00 | 1.63 | -20.90 | 107.30 | 78.88 | 248.80 | 0.9840 | 449.0 | 473.1 | |
| 0.00 | 2.39 | 0.00 | 6.14 | -21.06 | 106.63 | 78.21 | 248.60 | 0.9821 | 369.0 | 407.9 | |
| 5.20 | 168.41 | 15.67 | 451.55 | -23.10 | 108.24 | 79.82 | 246.63 | 0.9870 | -296.2 | 253.7 | |
| 14.48 | -3.00 | 38.72 | -3.00 | -23.04 | 106.89 | 78.47 | 246.60 | 0.9833 | 560.2 | 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. | |