| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.92 | 33.80 | 4.40 | 21.26 | -21.02 | 310.96 | -26.10 | 138.29 | 0.6186 | -117.8 | -110.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.04 | 0.00 | 1.24 | -20.86 | 314.94 | -22.12 | 142.62 | 0.5819 | 580.0 | 405.7 | |
| 0.00 | 1.51 | 0.00 | 0.92 | -19.89 | 313.95 | -23.12 | 140.30 | 0.5803 | 706.0 | 541.1 | |
| 0.00 | 0.53 | 0.00 | 0.32 | -19.32 | 313.41 | -23.66 | 138.98 | 0.5792 | 510.0 | 520.8 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -19.05 | 313.45 | -23.62 | 138.70 | 0.5760 | 852.0 | 747.2 | |
| 0.00 | 2.93 | 0.00 | 1.77 | -18.98 | 313.36 | -23.71 | 138.52 | 0.5763 | 770.0 | 664.7 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -18.79 | 313.14 | -23.93 | 138.03 | 0.5763 | 750.0 | 576.1 | |
| 1.24 | 3.02 | 0.76 | 1.85 | -20.13 | 312.61 | -24.46 | 139.01 | 0.5949 | 711.4 | 500.0 | |
| 0.62 | 1.95 | 0.40 | 1.24 | -21.69 | 310.28 | -26.79 | 138.27 | 0.6314 | -825.7 | -764.3 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -22.12 | 310.01 | -27.06 | 138.47 | 0.6379 | -339.0 | -331.5 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -21.29 | 310.07 | -27.00 | 137.60 | 0.6296 | -742.0 | -630.6 | |
| 0.98 | 2.93 | 0.62 | 1.86 | -21.06 | 310.04 | -27.03 | 137.30 | 0.6275 | -889.7 | -713.2 | |
| 0.00 | 3.73 | 0.00 | 2.40 | -22.14 | 309.67 | -27.39 | 138.15 | 0.6411 | -528.0 | -435.2 | |
| 0.00 | 1.15 | 0.00 | 0.74 | -21.83 | 309.74 | -27.33 | 137.87 | 0.6376 | -501.0 | -460.7 | |
| 0.00 | 0.89 | 0.00 | 0.57 | -22.05 | 309.44 | -27.63 | 137.81 | 0.6424 | -603.0 | -446.2 | |
| 2.66 | 7.89 | 1.71 | 5.07 | -21.64 | 309.49 | -27.58 | 137.40 | 0.6381 | -824.8 | -609.0 | |
| 1.42 | -15.00 | 0.91 | -15.00 | -21.58 | 309.24 | -27.83 | 137.09 | 0.6398 | -639.9 | 999999 | |
| 0.00 | 1.77 | 0.00 | 1.14 | -21.86 | 309.15 | -27.92 | 137.31 | 0.6432 | -345.0 | -300.4 | |
| 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. | |