SDO HMI 2014-05-23 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.93 | 52.68 | 9.19 | 28.48 | -13.63 | 135.71 | 20.47 | 238.46 | 0.4002 | 96.5 | -79.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.95 | 9.82 | 3.25 | 5.36 | -13.47 | 137.51 | 22.28 | 240.89 | 0.4237 | 934.7 | 719.2 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -13.10 | 137.21 | 21.97 | 241.38 | 0.4169 | 471.0 | 540.5 | |
| 0.00 | 1.98 | 0.00 | 1.08 | -13.65 | 137.23 | 21.99 | 240.20 | 0.4211 | 989.0 | 817.0 | |
| 4.32 | 7.84 | 2.35 | 4.26 | -13.10 | 136.91 | 21.67 | 241.06 | 0.4127 | 1109.5 | 835.0 | |
| 2.70 | 4.32 | 1.47 | 2.36 | -13.91 | 136.92 | 21.68 | 239.33 | 0.4187 | 965.4 | 737.7 | |
| 0.00 | 2.79 | 0.00 | 1.52 | -14.38 | 136.59 | 21.36 | 237.98 | 0.4178 | 1013.0 | 855.6 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -14.08 | 135.46 | 20.22 | 237.30 | 0.4001 | -714.0 | -608.2 | |
| 0.90 | 3.87 | 0.48 | 2.08 | -13.74 | 134.53 | 19.29 | 236.88 | 0.3849 | -790.1 | -558.0 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -13.15 | 134.42 | 19.18 | 238.07 | 0.3786 | -791.0 | -511.5 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -13.40 | 134.37 | 19.13 | 237.44 | 0.3799 | -724.0 | -527.9 | |
| 0.72 | 14.95 | 0.39 | 7.99 | -13.87 | 134.05 | 18.81 | 235.95 | 0.3794 | -996.2 | -786.3 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -14.12 | 133.93 | 18.70 | 235.24 | 0.3801 | -779.0 | -600.6 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -14.68 | 133.95 | 18.71 | 234.02 | 0.3852 | -738.0 | -606.0 | |
| 2.34 | -11.00 | 1.25 | -11.00 | -13.53 | 133.72 | 18.49 | 236.29 | 0.3722 | -1108.8 | 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. | |