| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.09 | 227.53 | 27.03 | 133.55 | 9.22 | 357.27 | -31.15 | 71.94 | 0.5391 | -771.2 | -296.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.16 | 188.94 | 19.95 | 110.37 | 9.39 | 357.79 | -30.63 | 71.40 | 0.5325 | -1162.8 | -405.6 | |
| 4.09 | -1.00 | 2.40 | -1.00 | 9.06 | 357.23 | -31.19 | 72.27 | 0.5390 | -732.7 | 999999 | |
| 0.00 | 3.75 | 0.00 | 2.20 | 8.49 | 357.07 | -31.35 | 73.37 | 0.5391 | -685.0 | -592.8 | |
| 3.07 | 4.26 | 1.81 | 2.51 | 8.88 | 356.86 | -31.56 | 72.77 | 0.5435 | -684.9 | -576.7 | |
| 0.00 | 1.79 | 0.00 | 1.06 | 9.45 | 356.73 | -31.69 | 71.82 | 0.5475 | -543.0 | -422.1 | |
| 0.00 | 1.19 | 0.00 | 0.71 | 8.77 | 356.34 | -32.08 | 73.21 | 0.5504 | -642.0 | -511.4 | |
| 0.00 | 0.94 | 0.00 | 0.56 | 8.50 | 355.38 | -33.04 | 74.09 | 0.5629 | -643.0 | -490.0 | |
| 2.39 | 5.45 | 1.43 | 3.27 | 8.80 | 355.27 | -33.14 | 73.62 | 0.5654 | -727.5 | -547.2 | |
| 1.36 | 13.63 | 0.82 | 8.24 | 8.30 | 354.32 | -34.10 | 74.86 | 0.5769 | 781.0 | 696.4 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 8.36 | 354.10 | -34.32 | 74.84 | 0.5802 | 798.0 | 698.5 | |
| 1.02 | 3.32 | 0.62 | 2.03 | 8.66 | 353.77 | -34.64 | 74.46 | 0.5856 | 941.8 | 807.5 | |
| 0.00 | 2.13 | 0.00 | 1.30 | 8.12 | 353.76 | -34.66 | 75.37 | 0.5841 | 654.0 | 538.6 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 8.69 | 353.48 | -34.94 | 74.52 | 0.5897 | 828.0 | 702.3 | |
| 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. | |