| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.47 | 0.00 | 11.71 | -5.04 | 138.78 | -21.77 | 117.76 | 0.4192 | -842.4 | -712.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.75 | -4.30 | 140.83 | -19.71 | 118.57 | 0.3846 | -824.0 | -624.6 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -4.63 | 140.05 | -20.49 | 118.36 | 0.3982 | -1020.0 | -894.4 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -4.56 | 139.70 | -20.84 | 117.77 | 0.4025 | -892.0 | -826.0 | |
| 0.00 | 2.73 | 0.00 | 1.48 | -5.76 | 139.47 | -21.08 | 120.07 | 0.4152 | -1170.0 | -947.0 | |
| 0.00 | 1.94 | 0.00 | 1.05 | -5.55 | 139.34 | -21.20 | 119.49 | 0.4152 | -955.0 | -827.0 | |
| 0.00 | 2.55 | 0.00 | 1.38 | -3.87 | 139.37 | -21.17 | 115.87 | 0.4022 | -970.0 | -769.9 | |
| 0.00 | 1.67 | 0.00 | 0.90 | -3.63 | 139.31 | -21.23 | 115.26 | 0.4013 | -765.0 | -604.6 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -6.33 | 139.12 | -21.43 | 120.82 | 0.4246 | -817.0 | -717.7 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -4.06 | 139.20 | -21.34 | 116.10 | 0.4060 | -781.0 | -591.8 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -4.60 | 138.57 | -21.97 | 116.60 | 0.4189 | -672.0 | -502.5 | |
| 0.00 | 1.85 | 0.00 | 1.02 | -6.52 | 138.16 | -22.38 | 120.09 | 0.4390 | -780.0 | -624.4 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -5.97 | 136.18 | -24.36 | 116.91 | 0.4619 | -786.0 | -628.8 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -4.27 | 135.86 | -24.68 | 113.24 | 0.4551 | -708.0 | -603.8 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -5.11 | 135.63 | -24.92 | 114.70 | 0.4638 | -654.0 | -481.6 | |
| 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. | |