| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.43 | 423.23 | 137.13 | 935.76 | -13.98 | 93.93 | -75.14 | 106.13 | 0.9762 | 30.3 | -130.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.40 | 103.24 | 13.14 | 168.43 | -11.75 | 99.71 | -69.35 | 105.00 | 0.9499 | 698.4 | 264.9 | |
| 0.00 | 2.95 | 0.00 | 4.62 | -11.23 | 99.55 | -69.51 | 104.43 | 0.9501 | 49.0 | 71.4 | |
| 2.41 | -1.00 | 3.90 | -1.00 | -11.79 | 99.05 | -70.01 | 104.91 | 0.9533 | 496.8 | 999999 | |
| 10.36 | -1.00 | 17.52 | -1.00 | -12.16 | 98.36 | -70.70 | 105.15 | 0.9571 | 371.3 | 999999 | |
| 0.00 | 0.71 | 0.00 | 1.37 | -14.15 | 96.64 | -72.42 | 106.82 | 0.9669 | 363.0 | 360.2 | |
| 0.00 | 3.57 | 0.00 | 5.91 | -11.21 | 98.46 | -70.60 | 104.18 | 0.9556 | -210.0 | -164.7 | |
| 3.13 | -1.00 | 5.49 | -1.00 | -12.09 | 97.63 | -71.43 | 104.93 | 0.9605 | -111.7 | 999999 | |
| 0.00 | 0.80 | 0.00 | 1.37 | -11.48 | 98.02 | -71.05 | 104.38 | 0.9581 | -256.0 | -208.2 | |
| 3.39 | 310.17 | 7.98 | 750.68 | -15.55 | 93.84 | -75.22 | 107.68 | 0.9786 | 342.8 | -209.0 | |
| 0.00 | 1.52 | 0.00 | 2.83 | -12.41 | 96.60 | -72.46 | 105.04 | 0.9654 | -507.0 | -352.5 | |
| 0.00 | 0.27 | 0.00 | 0.55 | -13.74 | 95.57 | -73.49 | 106.19 | 0.9709 | -103.0 | -142.0 | |
| 4.29 | -9.00 | 10.24 | -9.00 | -15.34 | 93.69 | -75.38 | 107.44 | 0.9790 | 53.4 | 999999 | |
| 20.54 | -9.00 | 56.47 | -9.00 | -15.04 | 92.02 | -77.04 | 106.83 | 0.9841 | -190.6 | 999999 | |
| 9.91 | -9.00 | 22.39 | -9.00 | -12.29 | 93.75 | -75.32 | 104.38 | 0.9767 | -201.9 | 999999 | |
| 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. | |