| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.41 | 119.03 | 23.69 | 106.20 | 16.73 | 51.79 | 53.18 | 292.70 | 0.8329 | -444.2 | -276.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.40 | 97.65 | 3.10 | 88.01 | 16.68 | 52.80 | 54.19 | 292.32 | 0.8418 | -372.0 | -287.1 | |
| 0.00 | 1.25 | 0.00 | 1.15 | 17.19 | 52.75 | 54.14 | 292.92 | 0.8427 | 182.0 | 179.1 | |
| 9.67 | -1.00 | 8.72 | -1.00 | 16.91 | 52.25 | 53.64 | 292.75 | 0.8376 | -594.0 | 999999 | |
| 8.50 | -1.00 | 7.62 | -1.00 | 16.58 | 52.12 | 53.50 | 292.42 | 0.8356 | -814.0 | 999999 | |
| 1.79 | -1.00 | 1.59 | -1.00 | 16.56 | 51.63 | 53.02 | 292.54 | 0.8311 | -767.3 | 999999 | |
| 0.63 | -1.00 | 0.56 | -1.00 | 16.72 | 51.64 | 53.03 | 292.72 | 0.8317 | -775.3 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.01 | 16.02 | 51.05 | 52.44 | 292.10 | 0.8245 | -678.0 | -580.4 | |
| 0.00 | 2.15 | 0.00 | 1.87 | 16.28 | 51.05 | 52.43 | 292.40 | 0.8251 | -812.0 | -678.7 | |
| 0.00 | 0.98 | 0.00 | 0.85 | 16.00 | 50.58 | 51.97 | 292.22 | 0.8201 | -478.0 | -527.5 | |
| 2.42 | 6.35 | 2.10 | 5.53 | 16.77 | 50.72 | 52.11 | 293.08 | 0.8235 | -498.0 | -618.2 | |
| 0.00 | 1.79 | 0.00 | 1.52 | 15.56 | 50.17 | 51.56 | 291.84 | 0.8150 | 453.0 | 357.0 | |
| 0.00 | 1.88 | 0.00 | 1.62 | 16.66 | 50.31 | 51.70 | 293.08 | 0.8195 | -679.0 | -622.2 | |
| 0.00 | 1.16 | 0.00 | 0.95 | 16.29 | 47.99 | 49.37 | 293.46 | 0.7964 | 537.0 | 387.4 | |
| 0.00 | 0.72 | 0.00 | 0.61 | 19.39 | 48.68 | 50.07 | 296.87 | 0.8130 | -266.0 | -216.2 | |
| 0.00 | 0.81 | 0.00 | 0.67 | 18.32 | 47.99 | 49.38 | 295.87 | 0.8031 | -422.0 | -346.0 | |
| 0.00 | 0.90 | 0.00 | 0.70 | 17.02 | 45.71 | 47.09 | 295.22 | 0.7764 | 377.0 | 330.0 | |
| 0.00 | 0.98 | 0.00 | 0.75 | 16.61 | 44.33 | 45.72 | 295.28 | 0.7610 | 690.0 | 508.5 | |
| 0.00 | 1.25 | 0.00 | 0.96 | 17.59 | 44.60 | 45.99 | 296.37 | 0.7674 | 479.0 | 348.9 | |
| 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. | |