| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 88 | 4 | 49 | 13.19 | 351.10 | -24.87 | 66.75 | 0.4456 | -440.8 | 366.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 10 | 0 | 5 | 11.36 | 356.36 | -19.60 | 67.73 | 0.3570 | 1020.0 | 860.0 | |
| 0 | 14 | 0 | 8 | 15.16 | 355.30 | -20.67 | 59.54 | 0.3969 | 1076.0 | 830.4 | |
| 0 | 11 | 0 | 6 | 15.03 | 354.96 | -21.01 | 60.20 | 0.4007 | 859.0 | 832.9 | |
| 0 | 6 | 0 | 3 | 14.66 | 354.87 | -21.10 | 61.13 | 0.3994 | 951.0 | 787.6 | |
| 0 | 3 | 0 | 2 | 12.20 | 354.66 | -21.31 | 67.12 | 0.3872 | 538.0 | 420.1 | |
| 0 | 4 | 0 | 2 | 15.11 | 351.97 | -23.99 | 62.88 | 0.4429 | 658.0 | 516.1 | |
| 0 | 3 | 0 | 2 | 11.73 | 351.93 | -24.03 | 70.27 | 0.4254 | 586.0 | 480.7 | |
| 0 | 4 | 0 | 2 | 12.32 | 349.82 | -26.15 | 70.31 | 0.4592 | 574.0 | 545.3 | |
| 0 | 3 | 0 | 2 | 16.52 | 348.49 | -27.48 | 62.87 | 0.4991 | 599.0 | 525.1 | |
| 8 | 17 | 4 | 9 | 12.23 | 348.37 | -27.60 | 71.28 | 0.4800 | -1063.1 | -619.3 | |
| 0 | 4 | 0 | 2 | 11.98 | 347.99 | -27.98 | 71.99 | 0.4846 | -840.0 | -566.9 | |
| 0 | 3 | 0 | 2 | 12.42 | 347.80 | -28.17 | 71.21 | 0.4890 | -686.0 | -557.1 | |
| 0 | 2 | 0 | 1 | 10.17 | 338.55 | -37.42 | 78.31 | 0.6130 | 622.0 | 495.4 | |
| 0 | 4 | 0 | 3 | 9.83 | 335.32 | -40.65 | 79.39 | 0.6553 | 760.0 | 661.5 | |
| 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. | |