| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.07 | 0.00 | 10.54 | 7.59 | 336.15 | -18.50 | 86.52 | 0.3155 | -186.1 | -93.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.51 | 0.00 | 0.76 | 7.33 | 345.19 | -9.46 | 88.41 | 0.1639 | -705.0 | -665.6 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 6.69 | 344.89 | -9.76 | 92.21 | 0.1693 | -1025.0 | -804.8 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 8.38 | 343.49 | -11.16 | 83.00 | 0.1938 | -1011.0 | -866.7 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 8.92 | 343.38 | -11.27 | 80.31 | 0.1967 | -890.0 | -704.6 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 8.36 | 342.87 | -11.78 | 83.36 | 0.2043 | -742.0 | -546.5 | |
| 0.00 | 0.44 | 0.00 | 0.22 | 8.99 | 342.57 | -12.08 | 80.51 | 0.2105 | -789.0 | -623.0 | |
| 0.00 | 2.04 | 0.00 | 1.04 | 9.19 | 342.25 | -12.40 | 79.77 | 0.2163 | -603.0 | -597.2 | |
| 0.00 | 0.36 | 0.00 | 0.18 | 10.48 | 341.89 | -12.76 | 74.35 | 0.2266 | -505.0 | -647.8 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 10.94 | 339.09 | -15.56 | 75.04 | 0.2739 | -834.0 | -628.9 | |
| 0.00 | 0.71 | 0.00 | 0.37 | 8.60 | 336.62 | -18.03 | 84.22 | 0.3090 | -611.0 | -509.6 | |
| 0.00 | 1.07 | 0.00 | 0.56 | 4.15 | 335.40 | -19.25 | 97.92 | 0.3334 | -845.0 | -584.8 | |
| 0.00 | 1.86 | 0.00 | 0.98 | 4.95 | 335.13 | -19.53 | 95.41 | 0.3360 | 993.0 | 765.4 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 7.61 | 329.36 | -25.29 | 87.35 | 0.4257 | 738.0 | 616.9 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 8.00 | 328.83 | -25.82 | 86.42 | 0.4340 | 604.0 | 419.2 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 7.81 | 327.48 | -27.17 | 86.85 | 0.4550 | 819.0 | 698.7 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 8.19 | 327.18 | -27.47 | 86.03 | 0.4596 | 768.0 | 557.3 | |
| 0.00 | 1.33 | 0.00 | 0.74 | 7.72 | 327.01 | -27.64 | 87.03 | 0.4623 | 689.0 | 477.8 | |
| 0.00 | 0.98 | 0.00 | 0.55 | 3.98 | 326.52 | -28.13 | 94.96 | 0.4741 | 600.0 | 447.6 | |
| 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. | |