| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.51 | 34.28 | 1.81 | 17.58 | -8.35 | 8.92 | -14.57 | 99.48 | 0.2541 | 368.7 | 307.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.53 | -6.84 | 12.48 | -11.01 | 93.55 | 0.1908 | 1048.0 | 805.8 | |
| 0.00 | 2.11 | 0.00 | 1.07 | -9.02 | 12.08 | -11.41 | 104.34 | 0.2026 | 891.0 | 679.1 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -9.14 | 11.82 | -11.66 | 104.62 | 0.2072 | 745.0 | 652.3 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -8.07 | 11.33 | -12.15 | 99.19 | 0.2121 | 955.0 | 794.4 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.22 | 10.83 | -12.65 | 95.01 | 0.2192 | 779.0 | 602.3 | |
| 0.00 | 1.93 | 0.00 | 0.98 | -6.68 | 10.79 | -12.70 | 92.53 | 0.2196 | 964.0 | 808.5 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -6.62 | 10.60 | -12.88 | 92.22 | 0.2227 | 800.0 | 617.9 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -9.00 | 10.15 | -13.34 | 102.49 | 0.2344 | -691.0 | -543.1 | |
| 0.00 | 3.43 | 0.00 | 1.75 | -8.87 | 9.75 | -13.74 | 101.64 | 0.2407 | 400.0 | 434.8 | |
| 2.81 | 6.07 | 1.44 | 3.10 | -9.86 | 9.68 | -13.81 | 105.59 | 0.2453 | 1153.2 | 752.6 | |
| 0.00 | 3.34 | 0.00 | 1.71 | -9.34 | 9.39 | -14.10 | 103.27 | 0.2481 | 827.0 | 624.0 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -9.70 | 9.21 | -14.27 | 104.53 | 0.2522 | 690.0 | 569.9 | |
| 0.00 | 1.76 | 0.00 | 0.90 | -9.33 | 8.85 | -14.63 | 102.81 | 0.2568 | 888.0 | 677.0 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -7.94 | 8.63 | -14.86 | 97.32 | 0.2572 | 813.0 | 604.1 | |
| 0.00 | 2.46 | 0.00 | 1.28 | -7.15 | 5.44 | -18.05 | 93.82 | 0.3094 | -944.0 | -734.8 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -6.87 | 5.26 | -18.22 | 92.92 | 0.3123 | -904.0 | -727.0 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -6.71 | 4.15 | -19.33 | 92.39 | 0.3306 | -743.0 | -557.3 | |
| 0.70 | 2.37 | 0.37 | 1.25 | -6.67 | 3.77 | -19.72 | 92.25 | 0.3368 | -907.2 | -757.5 | |
| 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. | |