| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.45 | 387.28 | 36.58 | 203.96 | -18.14 | 352.15 | 9.88 | 208.75 | 0.3412 | 1104.9 | 444.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.64 | -19.45 | 354.91 | 12.63 | 212.83 | 0.3819 | -783.0 | -597.9 | |
| 47.40 | 292.82 | 24.93 | 153.95 | -17.84 | 352.35 | 10.07 | 209.63 | 0.3383 | 1427.1 | 468.4 | |
| 1.79 | -2.00 | 0.94 | -2.00 | -17.29 | 352.19 | 9.92 | 210.12 | 0.3292 | 1192.3 | 999999 | |
| 12.51 | 59.40 | 6.62 | 31.47 | -19.02 | 352.07 | 9.80 | 207.25 | 0.3528 | 1028.0 | 242.9 | |
| 1.28 | -2.00 | 0.67 | -2.00 | -17.41 | 351.95 | 9.67 | 209.32 | 0.3289 | 1143.9 | 999999 | |
| 5.02 | 10.89 | 2.65 | 5.74 | -18.74 | 351.42 | 9.15 | 206.07 | 0.3440 | 1078.5 | 801.3 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -15.15 | 350.85 | 8.57 | 210.17 | 0.2875 | -885.0 | -790.6 | |
| 1.45 | 13.36 | 0.77 | 7.07 | -19.58 | 350.87 | 8.59 | 203.64 | 0.3526 | 757.2 | 789.4 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -16.46 | 350.50 | 8.22 | 206.97 | 0.3038 | -781.0 | -590.9 | |
| 0.00 | 1.96 | 0.00 | 1.04 | -20.64 | 350.58 | 8.30 | 201.73 | 0.3666 | 642.0 | 581.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.89 | 350.44 | 8.17 | 202.24 | 0.3545 | 862.0 | 650.8 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -20.49 | 350.44 | 8.17 | 201.57 | 0.3634 | 946.0 | 745.6 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -22.93 | 346.91 | 4.63 | 191.18 | 0.3851 | 682.0 | 667.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -22.35 | 346.66 | 4.39 | 190.92 | 0.3753 | 861.0 | 648.8 | |
| 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. | |