| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.38 | 183.09 | 20.10 | 93.46 | -17.97 | 30.29 | 3.22 | 192.63 | 0.2438 | 226.9 | 154.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.43 | -15.38 | 33.19 | 6.12 | 208.24 | 0.2181 | 904.0 | 745.6 | |
| 23.04 | 105.35 | 11.78 | 53.87 | -18.04 | 31.56 | 4.49 | 197.46 | 0.2491 | 1321.3 | 518.5 | |
| 0.77 | -2.00 | 0.39 | -2.00 | -18.32 | 31.23 | 4.15 | 195.91 | 0.2519 | 982.1 | 999999 | |
| 0.00 | 5.36 | 0.00 | 2.73 | -17.35 | 31.05 | 3.98 | 196.41 | 0.2353 | 1102.0 | 972.0 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -18.20 | 30.44 | 3.37 | 193.15 | 0.2466 | 676.0 | 544.7 | |
| 0.00 | 2.47 | 0.00 | 1.26 | -18.32 | 30.23 | 3.16 | 192.23 | 0.2478 | 792.0 | 668.8 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -15.81 | 29.67 | 2.60 | 192.38 | 0.2041 | 757.0 | 642.3 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -17.53 | 29.60 | 2.52 | 190.45 | 0.2326 | -866.0 | -612.6 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -17.90 | 29.57 | 2.50 | 190.05 | 0.2386 | -966.0 | -852.7 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -18.29 | 29.11 | 2.04 | 187.98 | 0.2440 | -905.0 | -817.2 | |
| 0.00 | 2.72 | 0.00 | 1.39 | -17.96 | 29.01 | 1.94 | 187.81 | 0.2382 | -880.0 | -840.4 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -18.17 | 28.86 | 1.79 | 187.08 | 0.2414 | -868.0 | -656.9 | |
| 14.12 | 58.84 | 7.19 | 29.98 | -17.90 | 28.11 | 1.04 | 184.23 | 0.2356 | -1247.7 | -529.4 | |
| 1.45 | -13.00 | 0.74 | -13.00 | -18.20 | 27.93 | 0.86 | 183.40 | 0.2405 | -875.5 | 999999 | |
| 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. | |