| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.01 | 38.46 | 10.14 | 21.79 | -18.09 | 77.62 | -22.70 | 130.78 | 0.4858 | -168.8 | -333.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.57 | 7.68 | 3.63 | 4.24 | -17.68 | 80.80 | -19.52 | 134.10 | 0.4452 | 1007.0 | 828.2 | |
| 0.00 | 0.68 | 0.00 | 0.38 | -17.68 | 79.31 | -21.01 | 132.09 | 0.4622 | 750.0 | 649.8 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -17.46 | 79.24 | -21.08 | 131.63 | 0.4610 | 857.0 | 682.7 | |
| 1.71 | 3.84 | 0.96 | 2.15 | -17.22 | 78.20 | -22.12 | 129.91 | 0.4708 | 898.5 | 815.9 | |
| 0.00 | 1.71 | 0.00 | 0.97 | -18.37 | 77.54 | -22.77 | 131.05 | 0.4891 | -823.0 | -675.2 | |
| 0.00 | 0.68 | 0.00 | 0.39 | -18.28 | 77.22 | -23.10 | 130.52 | 0.4920 | -736.0 | -609.5 | |
| 1.62 | 13.14 | 0.92 | 7.51 | -18.59 | 76.94 | -23.38 | 130.70 | 0.4982 | -906.7 | -701.2 | |
| 2.99 | -7.00 | 1.71 | -7.00 | -18.59 | 76.77 | -23.55 | 130.51 | 0.5001 | -927.6 | 999999 | |
| 1.54 | 2.13 | 0.87 | 1.21 | -17.81 | 76.71 | -23.61 | 129.17 | 0.4938 | -876.2 | -669.7 | |
| 3.58 | -7.00 | 2.05 | -7.00 | -18.62 | 76.56 | -23.76 | 130.32 | 0.5028 | -754.0 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -17.63 | 76.36 | -23.95 | 128.48 | 0.4963 | -709.0 | -545.7 | |
| 0.00 | 4.09 | 0.00 | 2.35 | -18.10 | 75.68 | -24.64 | 128.51 | 0.5084 | -667.0 | -794.2 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -18.31 | 75.51 | -24.81 | 128.68 | 0.5123 | -678.0 | -502.4 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -18.85 | 75.29 | -25.03 | 129.30 | 0.5195 | -846.0 | -707.3 | |
| 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. | |