| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.77 | 350.60 | 31.64 | 218.08 | 17.89 | 166.33 | 29.87 | 308.40 | 0.6070 | -772.2 | -341.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.73 | 18.24 | 167.66 | 31.21 | 307.69 | 0.6241 | 156.0 | 143.4 | |
| 50.77 | 329.34 | 31.64 | 205.18 | 17.86 | 166.52 | 30.06 | 308.18 | 0.6088 | -1304.4 | -402.5 | |
| 0.00 | 1.42 | 0.00 | 0.87 | 17.46 | 164.81 | 28.36 | 309.21 | 0.5870 | -437.0 | -345.9 | |
| 0.00 | 2.05 | 0.00 | 1.24 | 17.35 | 164.40 | 27.94 | 309.45 | 0.5815 | 629.0 | 433.0 | |
| 0.00 | 1.07 | 0.00 | 0.65 | 18.32 | 164.21 | 27.75 | 310.97 | 0.5877 | 310.0 | 378.9 | |
| 0.00 | 1.60 | 0.00 | 0.97 | 17.57 | 163.51 | 27.05 | 310.65 | 0.5737 | 512.0 | 482.5 | |
| 0.00 | 2.13 | 0.00 | 1.29 | 17.85 | 163.13 | 26.67 | 311.43 | 0.5720 | 868.0 | 704.8 | |
| 0.00 | 1.24 | 0.00 | 0.75 | 18.43 | 162.90 | 26.45 | 312.45 | 0.5749 | 619.0 | 524.6 | |
| 0.00 | 2.67 | 0.00 | 1.61 | 18.19 | 162.69 | 26.23 | 312.36 | 0.5704 | 794.0 | 671.6 | |
| 0.00 | 2.76 | 0.00 | 1.67 | 18.69 | 162.70 | 26.24 | 313.01 | 0.5750 | 667.0 | 529.2 | |
| 0.00 | 1.78 | 0.00 | 1.07 | 18.02 | 162.37 | 25.92 | 312.45 | 0.5655 | 747.0 | 673.9 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 18.84 | 162.33 | 25.88 | 313.60 | 0.5726 | 676.0 | 576.8 | |
| 0.00 | 1.42 | 0.00 | 0.87 | 21.08 | 162.12 | 25.67 | 316.72 | 0.5918 | 543.0 | 431.4 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 19.37 | 161.57 | 25.12 | 315.14 | 0.5698 | 717.0 | 634.7 | |
| 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. | |