| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.92 | 42.11 | 12.71 | 24.50 | -17.91 | 77.96 | -26.23 | 126.68 | 0.5261 | 67.9 | -71.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.53 | 10.74 | 4.86 | 6.12 | -17.33 | 80.11 | -24.08 | 127.91 | 0.4956 | 984.8 | 795.4 | |
| 1.45 | 1.71 | 0.83 | 0.98 | -17.34 | 79.19 | -25.00 | 126.94 | 0.5067 | 834.9 | 766.0 | |
| 1.88 | 2.39 | 1.08 | 1.37 | -17.12 | 78.67 | -25.51 | 126.06 | 0.5112 | 800.5 | 703.7 | |
| 0.68 | 4.86 | 0.39 | 2.81 | -17.25 | 78.14 | -26.05 | 125.74 | 0.5187 | 1028.5 | 741.5 | |
| 0.43 | -4.00 | 0.25 | -4.00 | -17.22 | 78.04 | -26.15 | 125.59 | 0.5197 | 807.0 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.69 | -17.16 | 77.77 | -26.41 | 125.23 | 0.5225 | 633.0 | 434.8 | |
| 0.00 | 2.81 | 0.00 | 1.65 | -18.37 | 77.51 | -26.68 | 126.94 | 0.5352 | -950.0 | -801.5 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -18.78 | 77.33 | -26.85 | 127.41 | 0.5405 | -672.0 | -489.0 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -16.79 | 77.34 | -26.84 | 124.22 | 0.5249 | 658.0 | 574.2 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -18.18 | 76.98 | -27.20 | 126.14 | 0.5400 | -889.0 | -605.2 | |
| 1.79 | 13.22 | 1.06 | 7.81 | -18.65 | 76.86 | -27.32 | 126.77 | 0.5450 | -852.1 | -566.8 | |
| 0.68 | -11.00 | 0.40 | -11.00 | -18.56 | 76.67 | -27.51 | 126.45 | 0.5466 | -943.8 | 999999 | |
| 6.48 | -11.00 | 3.84 | -11.00 | -18.72 | 76.50 | -27.68 | 126.53 | 0.5498 | -780.7 | 999999 | |
| 0.00 | 1.79 | 0.00 | 1.07 | -18.56 | 75.47 | -28.72 | 125.38 | 0.5608 | -866.0 | -722.0 | |
| 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. | |