| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.48 | 43.21 | 6.58 | 22.80 | 17.35 | 41.72 | -8.75 | 24.87 | 0.3458 | -219.4 | -224.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.41 | 16.26 | 3.90 | 8.56 | 18.14 | 44.35 | -6.12 | 17.52 | 0.3384 | -1040.3 | -387.8 | |
| 0.00 | 2.98 | 0.00 | 1.57 | 17.82 | 44.14 | -6.34 | 18.40 | 0.3344 | -909.0 | -796.8 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 17.56 | 43.95 | -6.52 | 19.16 | 0.3314 | -880.0 | -774.9 | |
| 1.99 | 2.26 | 1.04 | 1.18 | 17.34 | 43.83 | -6.64 | 19.72 | 0.3286 | -1005.9 | -871.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.02 | 43.24 | -7.24 | 21.70 | 0.3272 | -875.0 | -557.7 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 16.19 | 41.73 | -8.74 | 26.80 | 0.3251 | -962.0 | -800.6 | |
| 0.00 | 4.97 | 0.00 | 2.60 | 15.78 | 40.73 | -9.75 | 30.02 | 0.3271 | -760.0 | -628.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 15.47 | 38.40 | -12.08 | 36.08 | 0.3439 | 872.0 | 626.7 | |
| 1.45 | 1.99 | 0.77 | 1.06 | 17.48 | 37.68 | -12.79 | 34.25 | 0.3769 | 830.2 | 798.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 17.19 | 37.57 | -12.90 | 34.94 | 0.3741 | 875.0 | 712.4 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 19.31 | 36.45 | -14.03 | 33.90 | 0.4119 | 808.0 | 567.1 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 15.57 | 36.64 | -13.83 | 39.61 | 0.3628 | 1000.0 | 824.4 | |
| 1.36 | 1.90 | 0.72 | 1.01 | 16.17 | 36.54 | -13.94 | 38.74 | 0.3713 | 937.9 | 864.0 | |
| 0.27 | 1.90 | 0.15 | 1.03 | 17.20 | 34.98 | -15.50 | 39.89 | 0.3997 | 853.7 | 793.6 | |
| 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. | |