| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.90 | 0.00 | 12.46 | 4.12 | 138.98 | 27.56 | 290.69 | 0.4953 | 99.9 | 71.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.82 | 4.75 | 142.04 | 30.62 | 289.72 | 0.5413 | -676.0 | -655.6 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 5.13 | 141.61 | 30.19 | 290.66 | 0.5373 | -752.0 | -628.2 | |
| 0.00 | 2.19 | 0.00 | 1.27 | 2.93 | 141.51 | 30.09 | 286.80 | 0.5251 | -753.0 | -611.6 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 4.82 | 141.14 | 29.72 | 290.44 | 0.5293 | -632.0 | -513.2 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 4.91 | 140.97 | 29.55 | 290.70 | 0.5274 | -711.0 | -613.9 | |
| 0.00 | 1.58 | 0.00 | 0.92 | 7.04 | 140.34 | 28.92 | 294.90 | 0.5312 | -671.0 | -527.9 | |
| 0.00 | 1.40 | 0.00 | 0.80 | 3.77 | 139.82 | 28.40 | 289.43 | 0.5053 | -441.0 | -394.5 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 5.97 | 139.18 | 27.75 | 293.93 | 0.5088 | -426.0 | -423.3 | |
| 0.00 | 1.31 | 0.00 | 0.74 | 3.01 | 138.64 | 27.22 | 288.79 | 0.4845 | 787.0 | 686.9 | |
| 0.00 | 1.58 | 0.00 | 0.88 | 2.32 | 137.52 | 26.10 | 288.19 | 0.4646 | 706.0 | 605.9 | |
| 0.00 | 1.66 | 0.00 | 0.93 | 2.37 | 137.35 | 25.93 | 288.42 | 0.4624 | 927.0 | 766.7 | |
| 0.00 | 0.53 | 0.00 | 0.30 | 4.65 | 137.39 | 25.97 | 292.93 | 0.4758 | 708.0 | 612.2 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 4.31 | 137.31 | 25.89 | 292.34 | 0.4727 | 850.0 | 793.5 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 4.00 | 137.23 | 25.81 | 291.80 | 0.4697 | 677.0 | 542.4 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 2.75 | 137.06 | 25.64 | 289.41 | 0.4601 | 786.0 | 628.3 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 3.75 | 137.06 | 25.64 | 291.44 | 0.4657 | 694.0 | 497.2 | |
| 0.00 | 1.66 | 0.00 | 0.93 | 5.19 | 135.98 | 24.56 | 295.24 | 0.4596 | 625.0 | 540.9 | |
| 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. | |