| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.20 | 72.89 | 18.31 | 39.08 | -19.48 | 51.32 | 12.70 | 213.09 | 0.3821 | 298.0 | 427.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.08 | 0.00 | 1.11 | -18.63 | 53.15 | 14.54 | 218.20 | 0.3862 | 931.0 | 743.1 | |
| 21.11 | 30.68 | 11.36 | 16.51 | -19.17 | 53.03 | 14.42 | 217.08 | 0.3917 | 1021.8 | 717.9 | |
| 0.00 | 6.14 | 0.00 | 3.29 | -18.79 | 52.63 | 14.02 | 216.96 | 0.3831 | 908.0 | 851.9 | |
| 0.00 | 4.96 | 0.00 | 2.67 | -19.37 | 52.38 | 13.77 | 215.54 | 0.3880 | 647.0 | 608.1 | |
| 0.00 | 3.16 | 0.00 | 1.69 | -18.54 | 52.22 | 13.60 | 216.57 | 0.3758 | 668.0 | 535.8 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -18.38 | 51.74 | 13.13 | 215.89 | 0.3693 | 992.0 | 753.3 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -19.79 | 50.96 | 12.35 | 212.06 | 0.3806 | -528.0 | -411.1 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -20.62 | 50.93 | 12.31 | 210.79 | 0.3916 | 772.0 | 605.4 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -20.36 | 50.84 | 12.23 | 210.98 | 0.3874 | 857.0 | 727.3 | |
| 2.62 | 17.23 | 1.39 | 9.16 | -19.57 | 49.04 | 10.42 | 208.24 | 0.3619 | -1024.5 | -736.3 | |
| 10.47 | -10.00 | 5.56 | -10.00 | -19.82 | 48.86 | 10.24 | 207.48 | 0.3641 | -1044.5 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -23.43 | 48.54 | 9.93 | 202.57 | 0.4139 | 726.0 | 609.4 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -21.99 | 42.73 | 4.11 | 190.55 | 0.3648 | -737.0 | -643.8 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -22.25 | 41.88 | 3.27 | 188.30 | 0.3667 | -877.0 | -624.0 | |
| 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. | |