| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.14 | 400.33 | 37.72 | 215.38 | 17.78 | 166.78 | 1.16 | 357.15 | 0.3908 | -681.9 | -362.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.10 | 369.16 | 5.98 | 198.56 | 18.02 | 167.62 | 2.00 | 355.16 | 0.3948 | -1058.0 | -434.8 | |
| 50.78 | -1.00 | 27.29 | -1.00 | 17.73 | 167.14 | 1.52 | 356.26 | 0.3895 | -1313.4 | 999999 | |
| 0.27 | -1.00 | 0.14 | -1.00 | 17.43 | 166.95 | 1.33 | 356.69 | 0.3845 | -1548.3 | 999999 | |
| 0.00 | 5.06 | 0.00 | 2.72 | 17.50 | 163.69 | -1.93 | 4.78 | 0.3864 | 848.0 | 774.9 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 17.14 | 163.60 | -2.02 | 5.09 | 0.3807 | 739.0 | 628.0 | |
| 0.00 | 3.73 | 0.00 | 2.01 | 17.80 | 163.47 | -2.15 | 5.26 | 0.3914 | 619.0 | 572.3 | |
| 0.00 | 0.62 | 0.00 | 0.34 | 18.03 | 162.77 | -2.85 | 6.88 | 0.3964 | 564.0 | 549.3 | |
| 0.00 | 1.60 | 0.00 | 0.86 | 18.39 | 162.54 | -3.08 | 7.30 | 0.4026 | 682.0 | 574.8 | |
| 0.00 | 1.60 | 0.00 | 0.87 | 19.22 | 162.17 | -3.44 | 7.86 | 0.4164 | 741.0 | 576.5 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 18.36 | 162.13 | -3.49 | 8.28 | 0.4030 | 842.0 | 649.6 | |
| 2.13 | 3.55 | 1.15 | 1.92 | 17.95 | 160.42 | -5.20 | 12.45 | 0.4014 | 795.0 | 554.2 | |
| 0.00 | 0.62 | 0.00 | 0.34 | 18.77 | 160.30 | -5.32 | 12.27 | 0.4146 | -603.0 | -595.1 | |
| 3.46 | 9.32 | 1.87 | 5.02 | 17.56 | 160.30 | -5.31 | 12.95 | 0.3957 | 1007.3 | 742.7 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 17.79 | 160.20 | -5.42 | 13.05 | 0.3997 | -23.0 | 53.2 | |
| 2.40 | -13.00 | 1.29 | -13.00 | 17.40 | 160.15 | -5.47 | 13.41 | 0.3937 | 979.4 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 14.78 | 160.03 | -5.59 | 15.53 | 0.3531 | 819.0 | 669.6 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 20.75 | 158.71 | -6.91 | 14.51 | 0.4507 | 742.0 | 659.8 | |
| 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. | |