| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.14 | 361.92 | 91.09 | 673.64 | -7.92 | 220.01 | -73.69 | 99.14 | 0.9628 | 294.0 | 32.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.05 | 295.53 | 68.68 | 504.26 | -8.39 | 221.64 | -72.06 | 99.77 | 0.9563 | 564.3 | 129.0 | |
| 4.27 | -1.00 | 7.58 | -1.00 | -8.02 | 220.46 | -73.25 | 99.26 | 0.9619 | -124.3 | 999999 | |
| 0.00 | 1.82 | 0.00 | 3.47 | -8.79 | 219.38 | -74.32 | 99.94 | 0.9672 | -508.0 | -502.0 | |
| 0.00 | 8.26 | 0.00 | 16.16 | -7.53 | 218.99 | -74.72 | 98.62 | 0.9683 | -443.0 | -351.8 | |
| 0.00 | 0.91 | 0.00 | 1.92 | -9.02 | 217.90 | -75.81 | 100.04 | 0.9734 | -342.0 | -302.4 | |
| 0.00 | 1.63 | 0.00 | 3.20 | -6.31 | 218.84 | -74.87 | 97.34 | 0.9685 | -429.0 | -402.0 | |
| 0.00 | 0.27 | 0.00 | 0.56 | -7.36 | 218.22 | -75.48 | 98.37 | 0.9715 | -437.0 | -433.7 | |
| 0.00 | 0.82 | 0.00 | 1.65 | -6.98 | 218.41 | -75.29 | 97.99 | 0.9706 | -381.0 | -331.7 | |
| 3.00 | 25.34 | 6.84 | 59.78 | -6.20 | 216.69 | -77.01 | 97.05 | 0.9771 | -513.6 | -519.2 | |
| 0.00 | 5.45 | 0.00 | 14.12 | -8.13 | 215.24 | -78.46 | 98.90 | 0.9826 | -454.0 | -295.9 | |
| 0.00 | 0.73 | 0.00 | 1.92 | -7.10 | 215.00 | -78.71 | 97.83 | 0.9831 | -402.0 | -399.8 | |
| 0.00 | 0.73 | 0.00 | 1.94 | -6.76 | 214.89 | -78.82 | 97.48 | 0.9834 | -360.0 | -356.1 | |
| 2.82 | 5.54 | 7.99 | 15.75 | -6.46 | 214.24 | -79.46 | 97.12 | 0.9853 | -137.4 | -37.5 | |
| 0.00 | 14.89 | 0.00 | 48.91 | -6.23 | 212.72 | -80.98 | 96.78 | 0.9894 | 268.0 | 144.6 | |
| 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. | |