| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.29 | 0.00 | 11.91 | 13.45 | 56.60 | 11.49 | 306.56 | 0.2374 | 356.9 | 299.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.42 | 13.46 | 67.43 | 22.32 | 290.15 | 0.3952 | -665.0 | -526.7 | |
| 0.00 | 2.54 | 0.00 | 1.36 | 11.64 | 66.90 | 21.79 | 285.92 | 0.3797 | -778.0 | -581.5 | |
| 0.00 | 2.10 | 0.00 | 1.10 | 18.38 | 60.67 | 15.56 | 310.33 | 0.3354 | -680.0 | -530.6 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 12.64 | 59.59 | 14.48 | 295.60 | 0.2718 | 678.0 | 676.4 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 15.65 | 59.21 | 14.10 | 305.70 | 0.2902 | -799.0 | -643.2 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 13.49 | 55.48 | 10.37 | 306.60 | 0.2191 | 844.0 | 702.5 | |
| 0.00 | 4.20 | 0.00 | 2.13 | 13.68 | 55.30 | 10.19 | 307.75 | 0.2185 | 474.0 | 578.4 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 13.42 | 54.67 | 9.56 | 308.50 | 0.2073 | 870.0 | 643.2 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 13.03 | 54.28 | 9.17 | 308.10 | 0.1981 | 917.0 | 746.1 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 13.21 | 52.82 | 7.71 | 313.57 | 0.1812 | 796.0 | 607.8 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 12.39 | 52.77 | 7.66 | 310.26 | 0.1713 | 821.0 | 586.2 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 12.55 | 52.71 | 7.60 | 311.15 | 0.1723 | 918.0 | 702.2 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 14.61 | 51.94 | 6.83 | 322.21 | 0.1886 | 700.0 | 542.1 | |
| 0.00 | 3.50 | 0.00 | 1.75 | 11.49 | 50.83 | 5.73 | 313.90 | 0.1363 | 900.0 | 740.7 | |
| 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. | |