| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.78 | 252.85 | 26.32 | 162.52 | 5.79 | 44.82 | -38.20 | 75.67 | 0.6370 | -1032.0 | -328.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.93 | 0.00 | 0.50 | 12.74 | 70.03 | -12.99 | 37.56 | 0.3612 | -605.0 | -611.0 | |
| 0.00 | 2.12 | 0.00 | 1.13 | 9.55 | 65.81 | -17.21 | 51.74 | 0.3732 | -935.0 | -671.0 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 12.05 | 64.49 | -18.53 | 48.83 | 0.4147 | -626.0 | -437.8 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 12.01 | 61.34 | -21.67 | 53.24 | 0.4528 | -735.0 | -600.3 | |
| 0.00 | 0.93 | 0.00 | 0.52 | 10.29 | 59.76 | -23.26 | 58.30 | 0.4586 | -891.0 | -781.9 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 10.30 | 59.40 | -23.62 | 58.66 | 0.4635 | -841.0 | -703.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | 8.29 | 52.47 | -30.55 | 68.10 | 0.5442 | -645.0 | -446.0 | |
| 0.00 | 3.06 | 0.00 | 1.92 | 11.64 | 48.17 | -34.85 | 65.39 | 0.6178 | -449.0 | -510.3 | |
| 0.00 | 0.93 | 0.00 | 0.59 | 11.54 | 47.71 | -35.31 | 65.82 | 0.6231 | -631.0 | -456.5 | |
| 39.00 | 235.63 | 25.16 | 152.22 | 5.62 | 44.29 | -38.73 | 76.38 | 0.6430 | -1287.1 | -324.4 | |
| 1.78 | -10.00 | 1.16 | -10.00 | 5.34 | 43.89 | -39.13 | 76.94 | 0.6473 | -814.4 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.93 | 3.02 | 43.80 | -39.22 | 80.51 | 0.6425 | 472.0 | 511.7 | |
| 0.00 | 1.19 | 0.00 | 0.81 | 7.08 | 41.27 | -41.75 | 75.28 | 0.6856 | -447.0 | -387.1 | |
| 0.00 | 1.70 | 0.00 | 1.14 | -1.19 | 40.73 | -42.29 | 87.45 | 0.6758 | 113.0 | 186.0 | |
| 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. | |