| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.90 | 222.42 | 23.21 | 120.38 | -11.82 | 178.27 | -15.18 | 140.65 | 0.4048 | 404.9 | 241.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.02 | 183.74 | 1.09 | 98.86 | -11.98 | 179.43 | -14.01 | 142.97 | 0.3950 | 919.4 | 429.3 | |
| 0.00 | 1.49 | 0.00 | 0.81 | -12.24 | 179.42 | -14.02 | 143.34 | 0.3983 | 624.0 | 449.9 | |
| 33.32 | -1.00 | 17.93 | -1.00 | -11.55 | 179.11 | -14.34 | 141.65 | 0.3927 | 1242.4 | 999999 | |
| 1.67 | -1.00 | 0.91 | -1.00 | -12.23 | 178.47 | -14.98 | 141.51 | 0.4075 | 702.6 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -12.49 | 177.18 | -16.27 | 139.60 | 0.4237 | -601.0 | -395.1 | |
| 0.00 | 2.11 | 0.00 | 1.16 | -12.73 | 176.94 | -16.51 | 139.54 | 0.4289 | -767.0 | -551.5 | |
| 1.23 | 3.96 | 0.68 | 2.17 | -12.80 | 176.61 | -16.83 | 139.10 | 0.4331 | -905.5 | -588.9 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -14.61 | 174.36 | -19.09 | 138.23 | 0.4770 | -502.0 | -420.8 | |
| 0.00 | 2.20 | 0.00 | 1.24 | -14.58 | 174.20 | -19.25 | 137.96 | 0.4784 | -589.0 | -335.2 | |
| 0.00 | 1.67 | 0.00 | 0.93 | -12.09 | 174.37 | -19.07 | 134.40 | 0.4491 | -725.0 | -621.1 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -14.08 | 173.98 | -19.47 | 136.90 | 0.4750 | -806.0 | -595.0 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -14.09 | 173.65 | -19.80 | 136.44 | 0.4786 | -804.0 | -717.1 | |
| 3.08 | 5.89 | 1.72 | 3.29 | -12.56 | 173.62 | -19.83 | 134.05 | 0.4626 | -1015.7 | -814.6 | |
| 1.58 | 8.09 | 0.88 | 4.50 | -12.09 | 173.65 | -19.79 | 133.34 | 0.4571 | -1088.2 | -764.3 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -13.36 | 173.42 | -20.03 | 135.02 | 0.4733 | -851.0 | -716.5 | |
| 0.00 | 3.25 | 0.00 | 1.82 | -13.05 | 173.38 | -20.06 | 134.47 | 0.4703 | -965.0 | -674.7 | |
| 0.00 | 3.69 | 0.00 | 2.07 | -12.69 | 172.92 | -20.53 | 133.26 | 0.4716 | -760.0 | -481.5 | |
| 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. | |