| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.79 | 43.96 | 6.01 | 22.42 | 6.03 | 11.74 | 2.68 | 348.81 | 0.2375 | 97.0 | 101.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.58 | 4.31 | 18.40 | 9.34 | 320.80 | 0.2572 | 724.0 | 626.0 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 6.22 | 17.67 | 8.61 | 327.22 | 0.2762 | 705.0 | 571.2 | |
| 2.34 | 4.60 | 1.20 | 2.35 | 5.95 | 13.87 | 4.81 | 339.88 | 0.2435 | -1120.3 | -750.3 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 5.92 | 13.63 | 4.57 | 340.77 | 0.2416 | -931.0 | -732.5 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 6.22 | 13.51 | 4.45 | 341.62 | 0.2458 | -946.0 | -755.2 | |
| 2.51 | 4.60 | 1.29 | 2.35 | 6.74 | 13.12 | 4.07 | 343.72 | 0.2523 | -1101.0 | -836.4 | |
| 0.61 | 3.38 | 0.31 | 1.72 | 5.91 | 12.94 | 3.88 | 343.50 | 0.2379 | -938.4 | -731.2 | |
| 0.00 | 2.25 | 0.00 | 1.15 | 7.35 | 11.42 | 2.36 | 350.78 | 0.2560 | -1011.0 | -812.6 | |
| 0.00 | 3.47 | 0.00 | 1.76 | 5.17 | 10.83 | 1.78 | 351.81 | 0.2178 | 1246.0 | 989.7 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 5.29 | 10.63 | 1.57 | 352.83 | 0.2194 | 804.0 | 690.8 | |
| 0.52 | 1.65 | 0.26 | 0.84 | 5.60 | 10.39 | 1.33 | 354.06 | 0.2241 | 1096.5 | 910.5 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 5.75 | 10.39 | 1.33 | 354.12 | 0.2267 | 769.0 | 662.4 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 7.56 | 10.12 | 1.07 | 355.86 | 0.2570 | -895.0 | -693.5 | |
| 5.81 | 14.39 | 2.95 | 7.32 | 5.87 | 9.88 | 0.82 | 356.39 | 0.2281 | 1103.5 | 789.2 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 6.97 | 9.88 | 0.83 | 356.66 | 0.2469 | 639.0 | 462.0 | |
| 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. | |