| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.36 | 319.99 | 39.70 | 252.87 | 31.25 | 189.91 | -39.65 | 44.53 | 0.7804 | -1028.3 | -286.1 | |
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back to the solar disc SDO HMI 2011-01-02 22:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.42 | 0.00 | 0.36 | 34.97 | 188.70 | -40.87 | 41.46 | 0.8120 | 484.0 | 431.4 | |
| 49.00 | 318.81 | 38.62 | 251.89 | 31.25 | 189.93 | -39.63 | 44.51 | 0.7802 | -1100.9 | -287.4 | |
| 1.36 | -2.00 | 1.08 | -2.00 | 30.96 | 189.31 | -40.25 | 45.20 | 0.7831 | -552.1 | 999999 | |
| 0.00 | 0.76 | 0.00 | 0.62 | 30.85 | 187.59 | -41.98 | 46.36 | 0.7957 | -253.0 | -255.8 | |
| 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. | |