| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.14 | 196.47 | 21.67 | 100.91 | -17.92 | 30.34 | 7.10 | 206.41 | 0.2645 | 516.9 | 51.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.50 | 113.46 | 11.08 | 58.42 | -18.11 | 31.62 | 8.38 | 210.20 | 0.2767 | 1251.3 | 468.8 | |
| 4.42 | -1.00 | 2.27 | -1.00 | -17.39 | 31.21 | 7.97 | 210.40 | 0.2628 | 1179.4 | 999999 | |
| 4.76 | -1.00 | 2.44 | -1.00 | -17.66 | 31.19 | 7.96 | 209.80 | 0.2666 | 1171.7 | 999999 | |
| 1.78 | 5.01 | 0.92 | 2.58 | -18.18 | 30.97 | 7.73 | 208.12 | 0.2723 | 944.6 | 745.1 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -17.09 | 30.73 | 7.50 | 209.49 | 0.2545 | 868.0 | 697.7 | |
| 0.00 | 3.74 | 0.00 | 1.92 | -17.54 | 30.60 | 7.36 | 208.15 | 0.2600 | 826.0 | 632.8 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -18.03 | 30.46 | 7.22 | 206.82 | 0.2662 | 807.0 | 606.2 | |
| 0.00 | 2.29 | 0.00 | 1.18 | -18.30 | 30.35 | 7.11 | 205.98 | 0.2694 | 840.0 | 746.7 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -18.15 | 30.12 | 6.88 | 205.52 | 0.2655 | 554.0 | 463.4 | |
| 0.00 | 3.91 | 0.00 | 2.00 | -17.46 | 29.44 | 6.20 | 204.45 | 0.2501 | -903.0 | -839.4 | |
| 5.18 | 10.62 | 2.66 | 5.44 | -17.89 | 29.39 | 6.16 | 203.57 | 0.2563 | -1043.6 | -694.2 | |
| 0.00 | 2.29 | 0.00 | 1.17 | -17.80 | 28.99 | 5.75 | 202.32 | 0.2523 | -1171.0 | -923.4 | |
| 0.00 | 3.40 | 0.00 | 1.74 | -18.13 | 28.94 | 5.70 | 201.62 | 0.2572 | -827.0 | -805.5 | |
| 4.50 | 47.42 | 2.30 | 24.24 | -17.89 | 27.90 | 4.66 | 198.30 | 0.2474 | -1369.5 | -659.9 | |
| 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. | |