| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.18 | 164.94 | 26.19 | 99.95 | -16.88 | 195.03 | 32.36 | 243.13 | 0.5760 | 88.8 | 0.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.35 | 0.00 | 0.86 | -19.27 | 198.10 | 35.43 | 241.20 | 0.6267 | 655.0 | 493.5 | |
| 0.90 | 76.44 | 0.56 | 47.42 | -18.28 | 197.08 | 34.41 | 242.13 | 0.6092 | 528.5 | 437.2 | |
| 11.24 | -2.00 | 6.97 | -2.00 | -17.81 | 196.82 | 34.15 | 242.70 | 0.6037 | 1020.1 | 999999 | |
| 5.31 | -2.00 | 3.30 | -2.00 | -18.12 | 196.85 | 34.18 | 242.23 | 0.6056 | 972.0 | 999999 | |
| 0.00 | 0.36 | 0.00 | 0.22 | -16.12 | 196.24 | 33.58 | 245.05 | 0.5882 | 161.0 | 122.2 | |
| 2.61 | -2.00 | 1.61 | -2.00 | -18.03 | 196.60 | 33.93 | 242.22 | 0.6021 | 1081.4 | 999999 | |
| 2.97 | -2.00 | 1.83 | -2.00 | -17.37 | 196.42 | 33.75 | 243.15 | 0.5965 | 961.8 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.66 | -16.98 | 195.84 | 33.17 | 243.45 | 0.5872 | 565.0 | 452.3 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -15.44 | 194.21 | 31.54 | 245.01 | 0.5585 | -409.0 | -348.1 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -17.44 | 194.46 | 31.79 | 241.86 | 0.5722 | 712.0 | 534.7 | |
| 9.71 | 83.64 | 5.74 | 49.56 | -15.61 | 193.32 | 30.65 | 244.18 | 0.5476 | -1100.8 | -404.3 | |
| 6.12 | -11.00 | 3.62 | -11.00 | -16.05 | 193.39 | 30.72 | 243.48 | 0.5509 | -1036.6 | 999999 | |
| 3.42 | -11.00 | 2.03 | -11.00 | -16.36 | 193.30 | 30.63 | 242.89 | 0.5513 | -832.9 | 999999 | |
| 0.90 | -11.00 | 0.53 | -11.00 | -16.30 | 193.07 | 30.40 | 242.83 | 0.5480 | -883.9 | 999999 | |
| 0.00 | 0.45 | 0.00 | 0.26 | -15.89 | 191.58 | 28.91 | 242.53 | 0.5262 | -711.0 | -596.4 | |
| 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. | |